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\Table{1}{ The results of photometry.}
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\rm No.&\rm ~BD &\rm ~HD &\alpha(1950)&\delta(1950)&\rms~Sp.& V~ & U\!-\!P & P\!-\!X & X\!-\!Y & Y\!-\!Z & Z\!-\!V & V\!-\!S & n \cr
\noalign{\vskip2mm\hrule\vskip2mm}
  1.\, & 37^\circ779 &\,        & 3\!^{\rm h}\!28\!^{\rm m}\!15\!^{\rm s}& 37^\circ\!33^\prime\!\!.1 & F3V   &      9.29 &  0.51 &  0.60 &  0.61 &  0.31 &  0.17 &  0.44 &\,  1 \cr
  2.\, & 37^\circ794 &\,   22114& 3\,31\,56& 37\,51.0 & B7III &      7.57 &  0.43 &  0.51 &  0.27 &  0.17 &  0.12 &  0.24 &\,  1 \cr
  3.\, & 37^\circ796 &\,        & 3\,32\,57& 37\,55.6 & A1V   &      9.83 &  0.62 &  0.85 &  0.45 &  0.26 &  0.14 &  0.30 &\,  1 \cr
  4.\, & 30^\circ556 &\,   22307& 3\,33\,30& 30\,54.6 & F2V   &      8.57 &  0.57 &  0.67 &  0.57 &  0.26 &  0.13 &  0.38 &\,  2 \cr
  5.\, & 31^\circ622 &\,        & 3\,33\,35& 31\,21.2 & K5III &      9.83 &  0.83 &  1.58 &  2.28 &  0.75 &  0.58 &  1.19 &\,  2 \cr
  6.\!\!^*& 36^\circ730 &\,        & 3\,33\,55& 37\,00.0 & A0V   &     10.50 &  0.75 &  0.83 &  0.47 &  0.30 &  0.14 &  0.35 &\,  2 \cr
  7.\, & 30^\circ557 &\,   22360& 3\,34\,01& 30\,57.6 & G9III &      7.75 &  0.61 &  0.95 &  1.29 &  0.50 &  0.31 &  0.76 &\,  2 \cr
  8.\, & 31^\circ624 &\,        & 3\,34\,05& 31\,25.7 & F0V   &     10.86 &  0.53 &  0.67 &  0.62 &  0.34 &  0.20 &  0.43 &\,  2 \cr
  9.\, & 36^\circ731 &\,        & 3\,34\,08& 37\,04.5 & B8.5V &      9.58 &  0.67 &  0.73 &  0.43 &  0.30 &  0.15 &  0.36 &\,  2 \cr
 10.\, & 30^\circ558 &\,   22418& 3\,34\,22& 30\,57.4 & F5V   &      6.88 &  0.52 &  0.56 &  0.62 &  0.30 &  0.15 &  0.42 &\,  2 \cr
 11.\, & 31^\circ625 &\,        & 3\,34\,28& 31\,27.3 & A6V   &      9.36 &  0.57 &  0.75 &  0.56 &  0.27 &  0.18 &  0.34 &\,  2 \cr
 12.\, &             &\,        & 3\,34\,42& 31\,21.6 & F5V   &     11.13 &  0.54 &  0.56 &  0.68 &  0.37 &  0.23 &  0.50 &\,  2 \cr
 13.\, & 30^\circ557 &\,        & 3\,35\,07& 30\,42.2 & F7V   &     10.57 &  0.50 &  0.58 &  0.72 &  0.38 &  0.21 &  0.55 &\,  2 \cr
 14.\, & 32^\circ649 &\,        & 3\,35\,33& 32\,42.6 & F0V   &     10.21 &  0.62 &  0.72 &  0.66 &  0.32 &  0.19 &  0.45 &\,  2 \cr
 15.\, & 31^\circ627 &\,        & 3\,35\,46& 32\,05.1 & G2V   &     10.47 &  0.45 &  0.58 &  0.84 &  0.37 &  0.25 &  0.50 &\,  2 \cr
 16.\, & 30^\circ560 &\,        & 3\,35\,47& 31\,14.2 & A8V   &     10.08 &  0.61 &  0.72 &  0.60 &  0.24 &  0.17 &  0.38 &\,  2 \cr
 17.\, &             &\,        & 3\,35\,49& 32\,04.4 & G2V &    11.49 &  0.50 &  0.59 &  0.86 &  0.37 &  0.29 &  0.51 &\,  2 \cr
 18.\, &             &\,        & 3\,35\,55& 32\,03.8 & F8V   &     11.24 &  0.53 &  0.59 &  0.77 &  0.38 &  0.27 &  0.49 &\,  2 \cr
 19.\, & 32^\circ651 &\,        & 3\,36\,15& 32\,23.7 & F0V   &      9.50 &  0.62 &  0.77 &  0.61 &  0.27 &  0.15 &  0.39 &\,  1 \cr
 20.\, & 37^\circ808 &\,        & 3\,36\,34& 37\,37.5 & A4:IV &      9.70 &  0.84 &  0.97 &  0.68 &  0.37 &  0.20 &  0.46 &\,  2 \cr
 21.\, &             &\,        & 3\,36\,37& 31\,26.7 & G2V   &     11.99 &  0.45 &  0.67 &  0.84 &  0.40 &  0.27 &  0.55 &\,  2 \cr
 22.\!\!^*& 31^\circ629 &\,        & 3\,36\,48& 31\,45.9 & B3:III:&     9.10 &  0.66 &  0.62 &  1.03 &  0.76 &  0.39 &  1.07 &\,  4 \cr
 23.\, & 30^\circ561 &\,        & 3\,36\,58& 31\,09.3 & F1V   &      9.88 &  0.60 &  0.70 &  0.66 &  0.29 &  0.20 &  0.45 &\,  2 \cr
 24.\, & 30^\circ562 &\,        & 3\,37\,25& 31\,09.3 & F7V   &     10.12 &  0.55 &  0.62 &  0.77 &  0.37 &  0.23 &  0.55 &\,  2 \cr
 25.\, & 31^\circ630 &\,   22781& 3\,37\,42& 31\,40.0 & K2V   &      8.79 &  0.45 &  0.82 &  1.16 &  0.30 &  0.36 &  0.71 &\,  1 \cr
 26.\, &             &\,        & 3\,37\,51& 31\,08.5 & G1V   &     11.14 &  0.58 &  0.69 &  1.03 &  0.45 &  0.32 &  0.76 &\,  2 \cr
 27.\, &             &\,        & 3\,37\,54& 31\,58.4 & F8III &     12.33 &  0.81 &  0.78 &  1.08 &  0.60 &  0.34 &  0.91 &\,  1 \cr
 28.\, & 31^\circ632 &\,        & 3\,37\,54& 31\,57.5 & A9V   &      9.49 &  0.60 &  0.76 &  0.58 &  0.27 &  0.17 &  0.38 &\,  2 \cr
 29.\, & 31^\circ633 &\,        & 3\,37\,58& 31\,26.3 & G7V   &     10.21 &  0.43 &  0.64 &  0.91 &  0.35 &  0.25 &  0.61 &\,  2 \cr
 30.\, & 30^\circ563 &\,        & 3\,38\,05& 31\,17.4 & F4IV-V &     9.92 &  0.55 &  0.61 &  0.72 &  0.33 &  0.21 &  0.50 &\,  2 \cr
 31.\, & 34^\circ712 &\,   22848& 3\,38\,11& 34\,14.2 & K1III &      7.81 &  0.56 &  0.98 &  1.47 &  0.50 &  0.37 &  0.68 &\,  1 \cr
 32.\, & 37^\circ814 &\,   22859& 3\,38\,28& 37\,25.7 & A0V   &      7.74 &  0.54 &  0.83 &  0.34 &  0.17 &  0.07 &  0.15 &\,  2 \cr
 33.\, & 31^\circ634 &\,        & 3\,38\,32& 31\,26.6 & A8V   &     10.14 &  0.59 &  0.76 &  0.54 &  0.27 &  0.17 &  0.34 &\,  2 \cr
 34.\, & 31^\circ635 &\,        & 3\,38\,44& 31\,35.2 & F7V   &     10.59 &  0.54 &  0.58 &  0.73 &  0.36 &  0.22 &  0.54 &\,  2 \cr
 35.\, & 31^\circ636 &\,        & 3\,38\,50& 32\,13.7 & G2V   &      9.98 &  0.46 &  0.58 &  0.80 &  0.34 &  0.21 &  0.52 &\,  2 \cr
 36.\!\!^*& 36^\circ735 &\,        & 3\,39\,03& 37\,06.5 & B8.5IV &     9.89 &  0.67 &  0.71 &  0.45 &  0.30 &  0.16 &  0.38 &\,  2 \cr
 37.\!\!^*& 36^\circ735 &\,        & 3\,39\,03& 37\,06.6 & G8III-IV & 10.12 &  0.66 &  1.00 &  1.53 &  0.63 &  0.35 &  0.90  &\,  2 \cr 
 38.\, &             &\,        & 3\,39\,04& 32\,48.1 & A4V   &     10.52 &  0.76 &  1.00 &  0.66 &  0.37 &  0.18 &  0.51 &\,  2 \cr
 39.\, & 31^\circ637 &\,        & 3\,39\,08& 31\,31.1 & F9V   &      9.00 &  0.48 &  0.56 &  0.72 &  0.32 &  0.22 &  0.50 &\,  2 \cr
 40.\, &             &\,        & 3\,39\,08& 31\,16.5 & G1V   &     12.10 &  0.56 &  0.65 &  0.94 &  0.48 &  0.29 &  0.66 &\,  2 \cr
 41.\, & 30^\circ564 &\,        & 3\,39\,11& 31\,00.6 & F2V   &      9.72 &  0.64 &  0.70 &  0.71 &  0.36 &  0.20 &  0.52 &\,  2 \cr
 42.\!\!^*& 33^\circ698 &\,   22951& 3\,39\,12& 33\,48.4 & B1V   &      4.97 &  0.15 &  0.17 &  0.19 &  0.17 &  0.06 &  0.17 &\,  3 \cr
 43.\, &             &\,        & 3\,39\,14& 31\,45.9 & K3.5V &     12.67 &  0.45 &  1.10 &  1.49 &  0.32 &  0.47 &  0.90 &\,  2 \cr
 44.\, & 31^\circ638 &\,        & 3\,39\,14& 32\,15.1 & G1V   &      9.66 &  0.48 &  0.65 &  0.81 &  0.34 &  0.23 &  0.54 &\,  3 \cr
 45.\, &             &\,        & 3\,39\,15& 31\,14.9 & K3III &     12.64 &  0.87 &  1.25 &  2.12 &  0.81 &  0.56 &  1.28 &\,  2 \cr
 46.\, &             &\,        & 3\,39\,16& 31\,48.3 & A6IV  &     12.40 &  0.93 &  1.10 &  0.96 &  0.55 &  0.30 &  0.79 &\,  1 \cr
 47.\, & 32^\circ659 &\,   22963& 3\,39\,18& 32\,46.9 & F4V   &      6.73 &  0.50 &  0.63 &  0.64 &  0.32 &  0.16 &  0.45 &\,  2 \cr
 48.\, &             &\,        & 3\,39\,24& 32\,13.8 & K2V   &     11.05 &  0.49 &  0.90 &  1.30 &  0.30 &  0.40 &  0.75 &\,  2 \cr
}}
\continued{1}
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\rm No.&\rm ~BD &\rm ~HD &\alpha(1950)&\delta(1950)&\rms~Sp.& V~ & U\!-\!P & P\!-\!X & X\!-\!Y & Y\!-\!Z & Z\!-\!V & V\!-\!S & n \cr
\noalign{\vskip2mm\hrule\vskip2mm}
 49.\, &             &\,        & 3\,39\,35& 32\,13.7 &  G1V   &     12.46 &  0.50 &  0.53 &  0.86 &  0.40 &  0.26 &  0.62 &\,  1 \cr
 50.\, & 32^\circ660 &\,   23027& 3\,39\,52& 33\,10.0 &  A5V   &      9.25 &  0.70 &  0.86 &  0.62 &  0.32 &  0.17 &  0.43 &\,  2 \cr
 51.\, & 31^\circ639 &\,   23040& 3\,39\,52& 31\,29.6 &  K4V   &      9.10 &  0.48 &  0.99 &  1.42 &  0.27 &  0.47 &  0.82 &\,  2 \cr
 52.\, & 31^\circ640 &\,        & 3\,39\,53& 31\,49.0 &  A3V   &     11.40 &  0.89 &  1.02 &  0.92 &  0.58 &  0.34 &  0.80 &\,  2 \cr
 53.\, & 33^\circ703 &\,        & 3\,40\,05& 33\,25.8 &  A1V   &     10.82 &  0.75 &  0.97 &  0.61 &  0.43 &  0.16 &  0.44 &\,  1 \cr
 54.\, &             &\,        & 3\,40\,08& 31\,27.2 &  G0V   &     11.97 &  0.55 &  0.69 &  0.95 &  0.51 &  0.30 &  0.74 &\,  2 \cr
 55.\, & 33^\circ704 &\,   23060& 3\,40\,13& 33\,57.5 &  B3V   &      7.44 &  0.26 &  0.34 &  0.28 &  0.19 &  0.09 &  0.23 &\,  2 \cr
 56.\, &             &\,        & 3\,40\,16& 32\,08.1 &  K0III &     12.76 &  0.84 &  1.00 &  1.72 &  0.73 &  0.47 &  1.11 &\,  2 \cr
 57.\, & 32^\circ661 &\,        & 3\,40\,32& 32\,28.1 &  G0V   &      9.07 &  0.46 &  0.55 &  0.74 &  0.31 &  0.19 &  0.51 &\,  2 \cr
 58.\, &             &\,        & 3\,40\,43& 32\,03.7 &  G2IV  &     12.75 &  0.63 &  0.78 &  1.21 &  0.57 &  0.38 &  0.96 &\,  2 \cr
 59.\, & 32^\circ662 &\,        & 3\,40\,46& 32\,28.4 &  F0V   &      9.27 &  0.60 &  0.70 &  0.66 &  0.31 &  0.18 &  0.44 &\,  2 \cr
 60.\, & 33^\circ706 &\,        & 3\,40\,48& 34\,01.9 &  B8V   &     10.16 &  0.54 &  0.64 &  0.39 &  0.24 &  0.12 &  0.32 &\,  2 \cr
 61.\, & 36^\circ741 &\,   23130& 3\,40\,48& 36\,43.2 &  A2V   &      8.85 &  0.56 &  0.85 &  0.44 &  0.20 &  0.10 &  0.20 &\,  2 \cr
 62.\, &             &\,        & 3\,40\,50& 32\,00.3 &  F9.5V &     11.34 &  0.52 &  0.66 &  0.85 &  0.40 &  0.26 &  0.64 &\,  2 \cr
 63.\!\!^*& 31^\circ641 &\,        & 3\,41\,00& 31\,57.9 &  A3V   &      9.89 &  0.71 &  0.92 &  0.60 &  0.32 &  0.18 &  0.40 &\,  5 \cr
 64.\, &             &\,        & 3\,41\,01& 31\,57.8 &  A3V   &     10.00 &  0.71 &  0.92 &  0.63 &  0.34 &  0.18 &  0.42 &\,  5 \cr
 65.\, &             &\,        & 3\,41\,01& 31\,29.5 &  K1IV-V &   13.10 &  0.50 &  1.00 &  1.33 &  0.60 &  0.40 &  0.89  &\,  2 \cr
 66.\, &             &\,        & 3\,41\,11& 32\,00.1 &  F2V   &     11 91 &  0.66 &  0.71 &  0.82 &  0.47 &  0.26 &  0.68 &\,  2 \cr
 67.\!\!^*& 31^\circ642 &\,   23180& 3\,41\,11& 32\,07.8 &  B1III &      3.83 &  0.20 &  0.23 &  0.24 &  0.17 &  0.08 &  0.20 &\,  2 \cr
 68.\, &             &\,        & 3\,41\,13& 31\,58.2 &  G0V   &     11.62 &  0.51 &  0.61 &  0.88 &  0.43 &  0.25 &  0.66 &\,  2 \cr
 69.\!\!^*&             &\,        & 3\,41\,16& 32\,01.6 &  F9Ve?  &     13.47 &  0.78 &  0.79 &  1.17 &  0.61 &  0.39 &  0.99 &\,  3 \cr
 70.\, &             &\,        & 3\,41\,16& 32\,00.8 &  F1:IV &     11.55 &  0.80 &  0.87 &  0.91 &  0.55 &  0.35 &  0.80 &\,  4 \cr
 71.\!\!^*& 35^\circ744 &\,   23204& 3\,41\,22& 35\,41.9 &  A1V   &      8.32 &  0.59 &  0.86 &  0.43 &  0.22 &  0.12 &  0.20 &\,  2 \cr
 72.\, &             &\,        & 3\,41\,22& 32\,17.2 &  A1V   &     11.68 &  0.88 &  1.05 &  0.80 &  0.52 &  0.31 &  0.67 &\,  2 \cr
 73.\, &             &\,        & 3\,41\,23& 32\,00.5 &  A4V   &     11.75 &  0.83 &  1.04 &  0.81 &  0.49 &  0.27 &  0.65 &\,  4 \cr
 74.\, &             &\,        & 3\,41\,23& 31\,57.0 &  A8III-IV & 10.60 &  0.95 &  1.03 &  0.90 &  0.52 &  0.33 &  0.72  &\,  4 \cr
 75.\, &             &\,        & 3\,41\,23& 31\,59.4 &  G3:Ve? &     13.92 &  0.48 &  0.88 &  1.15 &  0.56 &  0.51 &  1.10 &\,  2 \cr
 76.\, &             &\,        & 3\,41\,24& 31\,59.2 &  F8:Ve? &     13.34 &  0.88 &  0.84 &  1.19 &  0.66 &  0.48 &  1.14 &\,  2 \cr
 77.\!\!^*& 31^\circ643 &\,        & 3\,41\,26& 32\,00.4 &  B4.5V &      8.52 &  0.56 &  0.58 &  0.64 &  0.44 &  0.26 &  0.64 &\,  7 \cr
 78.\, &             &\,        & 3\,41\,27& 32\,00.7 &  A3IV  &     10.22 &  0.99 &  1.04 &  0.80 &  0.52 &  0.28 &  0.73 &\,  5 \cr
 79.\, &             &\,        & 3\,41\,29& 31\,57.4 &  G7IVe? &   12.94 &  0.74 &  1.02 &  1.47 &  0.81 &  0.53 &  1.22  &\,  3 \cr
 80.\, &             &\,        & 3\,41\,39& 32\,10.0 &  B8V   &     14.02 &  0.98 &  1.06 &  1.08 &  0.85 &  0.47 &  1.05 &\,  2 \cr
 81.\, &             &\,        & 3\,41\,40& 32\,16.8 &  G1V   &     13.77 &  0.68 &  0.69 &  1.15 &  0.64 &  0.36 &  0.94 &\,  2 \cr
 82.\, &             &\,        & 3\,41\,40& 32\,22.1 &  K5III &     12.74 &  1.20 &  1.27 &  2.74 &  0.96 &  0.81 &  1.64 &\,  3 \cr
 83.\, &             &\,        & 3\,41\,40& 32\,06.2 &  K5:Ve? &     13.95 &  0.75 &  1.34 &  1.83 &  0.34 &  0.61 &  1.03 &\,  2 \cr
 84.\, &             &\,        & 3\,41\,41& 32\,07.5 &  K3V   &     13.25 &  0.40 &  1.08 &  1.54 &  0.48 &  0.39 &  0.86 &\,  2 \cr
 85.\, &             &\,        & 3\,41\,42& 32\,09.9 &  B5V   &     11.23 &  0.57 &  0.65 &  0.89 &  0.61 &  0.37 &  0.94 &\,  1 \cr
 86.\, &             &\,        & 3\,41\,48& 32\,18.0 &  K2III &     12.81 &  1.07 &  1.68 &  2.10 &  0.93 &  0.67 &  1.45 &\,  2 \cr
 87.\, &             &\,        & 3\,41\,53& 31\,55.5 &  A7V   &     13.32 &  0.95 &  1.00 &  1.09 &  0.70 &  0.40 &  0.91 &\,  2 \cr
 88.\, & 30^\circ567 &\,        & 3\,41\,57& 30\,45.1 &  A0IV  &      9.88 &  0.82 &  0.87 &  0.56 &  0.37 &  0.20 &  0.45 &\,  2 \cr
 89.\, &             &\,        & 3\,41\,59& 32\,01.1 &  G0IVe? &     12.65 &  0.67 &  0.85 &  1.05 &  0.62 &  0.39 &  0.93 &\,  2 \cr
 90.\, & 30^\circ568 &\,        & 3\,41\,59& 30\,56.3 &  A7IV  &      9.51 &  0.76 &  0.88 &  0.62 &  0.31 &  0.16 &  0.41 &\,  1 \cr
 91.\, &             &\,        & 3\,42\,00& 32\,24.5 &  K3III &     13.34 &  1.10 &  1.47 &  2.21 &  0.96 &  0.61 &  1.47 &\,  2 \cr
 92.\, &             &\,        & 3\,42\,00& 31\,50.8 &  K0V:  &     13.09 &  0.61 &  0.90 &  1.48 &  0.62 &  0.35 &  1.01 &\,  2 \cr
 93.\, &             &\,        & 3\,42\,00& 30\,44.6 &  G5III &     10.77 &  0.73 &  0.94 &  1.36 &  0.72 &  0.38 &  1.03 &\,  2 \cr
 94.\, &             &\,        & 3\,42\,11& 32\,19.4 &  F6V   &     11.63 &  0.56 &  0.64 &  0.74 &  0.42 &  0.22 &  0.59 &\,  2 \cr
 95.\, &             &\,        & 3\,42\,15& 32\,28.4 &  A7m:  &     11.72 &  0.84 &  1.01 &  1.04 &  0.63 &  0.35 &  0.85 &\,  2 \cr
 96.\, & 31^\circ644 &\,   23322& 3\,42\,18& 32\,07.9 &  G9III-IV &  7.87 &  0.67 &  0.97 &  1.37 &  0.56 &  0.37 &  0.88  &\,  2 \cr
}}
\continued{1}
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\halign to \hsize{
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&\rms~#\hfil&
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\rm No.&\rm ~BD &\rm ~HD &\alpha(1950)&\delta(1950)&\rms~Sp.& V~ & U\!-\!P & P\!-\!X & X\!-\!Y & Y\!-\!Z & Z\!-\!V & V\!-\!S & n \cr
\noalign{\vskip2mm\hrule\vskip2mm}
 97.\!\!^*&             &\,        & 3\,42\,28& 32\,16.6 &  K5IV-Ve &   14.63 &  0.41 &  0.99 &  1.95 &  0.75 &  0.68 &  1.48 &\,  2 \cr
 98.\, &             &\,        & 3\,42\,29& 32\,17.7 &  G2IV-V &   11.97 &  0.55 &  0.67 &  0.97 &  0.46 &  0.29 &  0.69  &\,  2 \cr
 99.\, & 31^\circ645 &\,        & 3\,42\,30& 32\,17.1 &  B3V   &      9.13 &  0.49 &  0.52 &  0.65 &  0.50 &  0.23 &  0.64 &\,  3 \cr
100.\, & 33^\circ712 &\,        & 3\,42\,38& 33\,28.2 &  A4V   &     10.30 &  0.75 &  0.93 &  0.68 &  0.37 &  0.22 &  0.47 &\,  2 \cr
101.\, & 31^\circ646 &\,        & 3\,42\,40& 31\,51.7 &  A6V   &      9.71 &  0.73 &  0.86 &  0.61 &  0.32 &  0.16 &  0.45 &\,  4 \cr
102.\!\!^*&             &\,        & 3\,42\,40& 32\,14.9 &  F9IVe &     12.10 &  0.83 &  0.84 &  1.17 &  0.70 &  0.39 &  1.13 &\,  3 \cr
103.\, &             &\,        & 3\,42\,43& 32\,04.1 &  A2V   &     11.88 &  0.83 &  1.04 &  0.78 &  0.50 &  0.30 &  0.60 &\,  2 \cr
104.\, &             &\,        & 3\,42\,48& 32\,03.5 &  G2V   &     12.01 &  0.52 &  0.67 &  0.92 &  0.47 &  0.30 &  0.62 &\,  2 \cr
105.\, &             &\,        & 3\,43\,05& 32\,03.5 &  G5IV-V &   11.37 &  0.48 &  0.83 &  1.09 &  0.49 &  0.34 &  0.71  &\,  2 \cr
106.\!\!^*& 31^\circ647 &\,        & 3\,43\,15& 32\,06.0 &  A2V   &      9.64 &  0.64 &  0.86 &  0.47 &  0.23 &  0.12 &  0.27 &\,  3 \cr
107.\, & 33^\circ714 &\,        & 3\,43\,21& 33\,43.1 &  A4V   &     10.38 &  0.65 &  0.87 &  0.58 &  0.28 &  0.17 &  0.33 &\,  2 \cr
108.\, & 37^\circ827 &\,        & 3\,43\,25& 37\,47.1 &  A1V   &     11.32 &  0.59 &  0.96 &  0.59 &  0.28 &  0.20 &  0.35 &\,  1 \cr
109.\, & 31^\circ649 &\,   23478& 3\,43\,32& 32\,08.1 &  B3V   &      6.62 &  0.26 &  0.34 &  0.27 &  0.17 &  0.08 &  0.23 &\,  3 \cr
110.\, & 32^\circ665 &\,        & 3\,43\,38& 32\,27.0 &  F2V   &      9.28 &  0.70 &  0.78 &  0.73 &  0.38 &  0.22 &  0.57 &\,  2 \cr
111.\, & 37^\circ828 &\,        & 3\,43\,43& 37\,56.8 &  A5IV:   &      9.37 &  0.82 &  0.90 &  0.74 &  0.43 &  0.25 &  0.64 &\,  1 \cr
112.\, & 34^\circ730 &\,        & 3\,44\,15& 35\,09.5 &  F2V   &     10.30 &  0.55 &  0.65 &  0.65 &  0.32 &  0.20 &  0.45 &\,  1 \cr
113.\, & 34^\circ730 &\,        & 3\,44\,16& 35\,09.6 &  K5III: &     10.31 &  0.39 &  1.10 &  1.79 &  0.58 &  0.48 &  0.93 &\,  1 \cr
114.\, & 32^\circ666 &\,        & 3\,44\,17& 33\,10.2 &  B9.5III &    9.72 &  0.73 &  0.76 &  0.44 &  0.28 &  0.16 &  0.37 &\,  2 \cr
115.\, &             &\,        & 3\,44\,18& 33\,08.3 &  F8V   &     11.00 &  0.56 &  0.67 &  0.89 &  0.43 &  0.29 &  0.67 &\,  2 \cr
116.\, &             &\,        & 3\,44\,29& 33\,03.5 &  F5V   &     11.11 &  0.60 &  0.65 &  0.72 &  0.36 &  0.20 &  0.56 &\,  2 \cr
117.\!\!^*& 34^\circ732 &\,   23606& 3\,44\,35& 34\,51.8 &  B8.5V &      9.53 &  0.55 &  0.71 &  0.31 &  0.20 &  0.13 &  0.20 &\,  2 \cr
118.\!\!^*& 33^\circ717 &\,        & 3\,44\,41& 33\,26.8 &  B2V   &      6.53 &  0.24 &  0.30 &  0.25 &  0.19 &  0.10 &  0.22 &\,  2 \cr
119.\, & 31^\circ652 &\,   23699& 3\,45\,15& 31\,48.6 &  A8V   &      8.15 &  0.68 &  0.79 &  0.62 &  0.30 &  0.16 &  0.40 &\,  1 \cr
120.\, & 31^\circ653 &\,        & 3\,45\,21& 31\,09.0 &  A2.5IV &    10.39 &  0.85 &  0.95 &  0.58 &  0.33 &  0.19 &  0.44 &\,  2 \cr
121.\!\!^*& 31^\circ655 &\,   23802& 3\,45\,58& 32\,06.7 &  B6V   &      7.40 &  0.42 &  0.50 &  0.35 &  0.22 &  0.09 &  0.29 &\,  2 \cr
122.\, & 34^\circ739 &\,   23840& 3\,46\,16& 34\,46.0 &  B7V   &      8.47 &  0.47 &  0.60 &  0.27 &  0.17 &  0.11 &  0.15 &\,  2 \cr
123.\!\!^*& 32^\circ667 &\,   23848& 3\,46\,23& 32\,56.3 &  A2V   &      5.14 &  0.68 &  0.85 &  0.34 &  0.16 &  0.07 &  0.17 &\,  2 \cr
124.\, & 31^\circ657 &\,   23963& 3\,47\,20& 32\,16.8 &  B9V   &      9.48 &  0.61 &  0.71 &  0.37 &  0.21 &  0.10 &  0.24 &\,  2 \cr
125.\, & 31^\circ658 &\,   23974& 3\,47\,20& 31\,24.2 &  B6V   &      8.52 &  0.44 &  0.58 &  0.40 &  0.28 &  0.12 &  0.34 &\,  1 \cr
126.\, & 31^\circ659 &\,   24039& 3\,47\,50& 32\,01.2 &  A4.5IV &     9.23 &  0.74 &  0.95 &  0.59 &  0.32 &  0.16 &  0.37 &\,  3 \cr
127.\!\!^*& 32^\circ669 &\,   24038& 3\,47\,52& 32\,24.5 &  A6V   &      9.04 &  0.70 &  0.91 &  0.61 &  0.31 &  0.15 &  0.38 &\,  2 \cr
128.\, & 36^\circ763 &\,        & 3\,48\,02& 37\,03.3 &  A8V   &      9.07 &  0.57 &  0.70 &  0.56 &  0.26 &  0.15 &  0.35 &\,  2 \cr
129.\, & 34^\circ748 &\,        & 3\,48\,22& 34\,59.8 &  B9.5V &      9.73 &  0.61 &  0.80 &  0.36 &  0.21 &  0.12 &  0.18 &\,  2 \cr
130.\, & 34^\circ753 &\,        & 3\,48\,39& 34\,19.9 &  B8V   &      9.20 &  0.57 &  0.70 &  0.34 &  0.22 &  0.12 &  0.25 &\,  2 \cr
131.\, & 33^\circ727 &\,        & 3\,48\,40& 33\,50.6 &  K1III &      9.67 &  0.49 &  0.96 &  1.39 &  0.50 &  0.32 &  0.77 &\,  2 \cr
132.\, & 33^\circ728 &\,   24131& 3\,48\,42& 34\,12.6 &  B1V   &      5.75 &  0.16 &  0.19 &  0.19 &  0.16 &  0.09 &  0.18 &\,  2 \cr
133.\, & 30^\circ581 &\,        & 3\,48\,44& 31\,06.0 &  A0V   &     10.89 &  0.64 &  0.94 &  0.51 &  0.32 &  0.14 &  0.37 &\,  2 \cr
134.\, & 30^\circ582 &\,   24167& 3\,48\,57& 31\,01.2 &  A5V   &      6.18 &  0.64 &  0.80 &  0.46 &  0.20 &  0.10 &  0.25 &\,  2 \cr
135.\, & 32^\circ674 &\,        & 3\,49\,05& 33\,15.4 &  A5I-II &     8.92 &  1.25 &  0.84 &  0.52 &  0.38 &  0.20 &  0.55 &\,  2 \cr
136.\, & 33^\circ730 &\,   24190& 3\,49\,06& 34\,04.4 &  B2V   &      7.41 &  0.24 &  0.31 &  0.23 &  0.18 &  0.09 &  0.21 &\,  2 \cr
137.\, & 34^\circ755 &\,        & 3\,49\,12& 34\,18.9 &  B9.5V &      9.58 &  0.49 &  0.62 &  0.32 &  0.18 &  0.11 &  0.22 &\,  2 \cr
138.\, & 30^\circ584 &\,        & 3\,49\,13& 30\,59.4 &  A6V   &      9.64 &  0.78 &  0.91 &  0.65 &  0.39 &  0.17 &  0.47 &\,  2 \cr
139.\, & 32^\circ676 &\,        & 3\,49\,26& 32\,58.7 &  A0V   &      9.71 &  0.75 &  0.85 &  0.40 &  0.23 &  0.14 &  0.28 &\,  2 \cr
140.\, & 35^\circ757 &\,        & 3\,49\,27& 35\,37.5 &  A4V   &     10.09 &  0.71 &  0.85 &  0.55 &  0.27 &  0.17 &  0.36 &\,  2 \cr
141.\, & 31^\circ662 &\,   24222& 3\,49\,30& 32\,15.6 &  G7III &      6.70 &  0.57 &  0.83 &  1.11 &  0.44 &  0.28 &  0.65 &\,  1 \cr
142.\, & 34^\circ758 &\,   24242& 3\,49\,37& 34\,19.6 &  A1V   &      9.48 &  0.57 &  0.87 &  0.42 &  0.21 &  0.10 &  0.20 &\,  2 \cr
143.\, & 36^\circ769 &\,        & 3\,49\,38& 36\,42.4 &  B9.5V &      9.75 &  0.76 &  0.85 &  0.44 &  0.28 &  0.16 &  0.34 &\,  2 \cr
144.\, & 34^\circ759 &\,        & 3\,50\,05& 34\,45.7 &  A7IV  &     10.18 &  0.61 &  0.73 &  0.56 &  0.29 &  0.17 &  0.38 &\,  2 \cr
}}
\continued{1}
\vbox{\tabskip 33pt minus 33pt \baselineskip=10truept
\halign to \hsize{
\hfil$\scriptstyle#$&$\scriptstyle#$\hfil&$\scriptstyle#\hfil$&
\hfil$\scriptstyle#$\hfil&\hfil$\scriptstyle#$\hfil
&\rms~#\hfil&
\hfil$\scriptstyle#$&\hfil$\scriptstyle#$&\hfil$\scriptstyle#$&
\hfil$\scriptstyle#$&\hfil$\scriptstyle#$&\hfil$\scriptstyle#$&
\hfil$\scriptstyle#$&$\scriptstyle#$\cr
\noalign{\vskip2mm\hrule\vskip2mm}
\rm No.&\rm ~BD &\rm ~HD &\alpha(1950)&\delta(1950)&\rms~Sp.& V~ & U\!-\!P & P\!-\!X & X\!-\!Y & Y\!-\!Z & Z\!-\!V & V\!-\!S & n \cr
\noalign{\vskip2mm\hrule\vskip2mm}
145.\, & 35^\circ763 &\,   24300& 3\,50\,08& 35\,24.3 &  B5.5V &      8.65 &  0.37 &  0.51 &  0.25 &  0.17 &  0.10 &  0.18 &\,  2 \cr
146.\, & 35^\circ764 &\,        & 3\,50\,11& 35\,39.1 &  B7V   &      9.42 &  0.46 &  0.60 &  0.31 &  0.20 &  0.11 &  0.23 &\,  2 \cr
147.\!\!^*& 34^\circ761 &\,   24321& 3\,50\,19& 34\,54.7 &  B7V   &      8.80 &  0.42 &  0.57 &  0.30 &  0.19 &  0.10 &  0.21 &\,  2 \cr
148.\, & 32^\circ679 &\,   24322& 3\,50\,19& 32\,57.8 &  A3V   &      8.26 &  0.65 &  0.88 &  0.52 &  0.25 &  0.13 &  0.29 &\,  2 \cr
149.\!\!^*& 31^\circ666 &\,   24398& 3\,50\,59& 31\,44.2 &  B1Ib  &      2.85 &  0.22 &  0.21 &  0.25 &  0.22 &  0.10 &  0.24 &\,  2 \cr
150.\, & 32^\circ683 &\,   24411& 3\,51\,09& 32\,47.8 &  A2V   &      8.96 &  0.64 &  0.86 &  0.53 &  0.27 &  0.15 &  0.32 &\,  2 \cr
151.\, & 30^\circ589 &\,        & 3\,51\,13& 30\,51.1 &  A2V   &      9.49 &  0.75 &  0.91 &  0.62 &  0.40 &  0.19 &  0.47 &\,  2 \cr
152.\!\!^*& 34^\circ766 &\,        & 3\,52\,06& 34\,08.1 &  A1V   &      9.52 &  0.57 &  0.81 &  0.47 &  0.24 &  0.15 &  0.31 &\,  2 \cr
153.\!\!^*& 30^\circ591 &\,   24534& 3\,52\,15& 30\,54.0 &  O9.5ep &      6.10 &  0.15 &  0.13 &  0.27 &  0.25 &  0.10 &  0.39 &\,  3 \cr
154.\, & 34^\circ767 &\,   24583& 3\,52\,40& 34\,23.9 &  B7V   &      8.96 &  0.46 &  0.60 &  0.28 &  0.18 &  0.10 &  0.20 &\,  2 \cr
155.\!\!^*& 31^\circ669 &\,   24601& 3\,52\,45& 32\,00.6 &  B8V   &      8.60 &  0.54 &  0.66 &  0.36 &  0.23 &  0.11 &  0.28 &\,  2 \cr
156.\, & 33^\circ741 &\,        & 3\,52\,45& 34\,08.7 &  A0V   &      9.98 &  0.54 &  0.81 &  0.38 &  0.21 &  0.10 &  0.21 &\,  2 \cr
157.\, & 31^\circ670 &\,   24600& 3\,52\,49& 32\,01.1 &  B9.5V &      8.87 &  0.56 &  0.69 &  0.43 &  0.26 &  0.12 &  0.29 &\,  2 \cr
158.\, & 33^\circ743 &\,        & 3\,52\,57& 34\,15.1 &  A7IV: &      9.53 &  0.59 &  0.76 &  0.60 &  0.32 &  0.17 &  0.41 &\,  2 \cr
159.\!\!^*& 34^\circ768 &\,   24640& 3\,53\,15& 34\,56.1 &  B1V   &      5.46 &  0.18 &  0.24 &  0.18 &  0.15 &  0.08 &  0.16 &\,  2 \cr
160.\, & 35^\circ771 &\,   24664& 3\,53\,29& 35\,51.5 &  F8V   &      8.29 &  0.45 &  0.55 &  0.68 &  0.33 &  0.19 &  0.48 &\,  2 \cr
161.\, & 32^\circ691 &\,   24736& 3\,54\,09& 32\,44.6 &  B9V   &      8.55 &  0.58 &  0.73 &  0.34 &  0.21 &  0.12 &  0.22 &\,  2 \cr
162.\, & 35^\circ772 &\,        & 3\,54\,23& 35\,49.9 &  K3III &      9.09 &  0.62 &  1.22 &  1.83 &  0.64 &  0.44 &  0.96 &\,  1 \cr
163.\!\!^*& 35^\circ775 &\,        & 3\,55\,43& 35\,38.9 &  O8III &      4.02 &  0.11 &  0.08 &  0.19 &  0.17 &  0.09 &  0.24 &\,  2 \cr
164.\, & 32^\circ697 &\,   24913& 3\,55\,45& 32\,36.9 &  A1V   &      8.36 &  0.64 &  0.83 &  0.41 &  0.22 &  0.11 &  0.24 &\,  2 \cr
165.\, & 32^\circ698 &\,        & 3\,55\,58& 32\,34.8 &  A7:IV  &      9.85 &  0.75 &  0.85 &  0.69 &  0.31 &  0.18 &  0.44 &\,  1 \cr
166.\, & 31^\circ680 &\,        & 3\,56\,43& 31\,55.4 &  B6V   &      9.31 &  0.44 &  0.54 &  0.31 &  0.20 &  0.10 &  0.23 &\,  2 \cr
167.\, & 35^\circ781 &\,        & 3\,56\,49& 35\,39.1 &  A1V   &      9.90 &  0.64 &  0.88 &  0.47 &  0.25 &  0.15 &  0.30 &\,  2 \cr
168.\, & 32^\circ703 &\,   25143& 3\,57\,46& 32\,16.9 &  B8.5V &      8.53 &  0.49 &  0.64 &  0.34 &  0.20 &  0.08 &  0.22 &\,  2 \cr
169.\, & 34^\circ788 &\,        & 3\,58\,00& 35\,13.6 &  F5V   &     10.28 &  0.50 &  0.66 &  0.71 &  0.36 &  0.22 &  0.56 &\,  1 \cr
170.\, & 31^\circ686 &\,   25185& 3\,58\,15& 32\,07.8 &  A3V   &      8.86 &  0.71 &  0.90 &  0.51 &  0.27 &  0.13 &  0.31 &\,  2 \cr
171.\, & 34^\circ790 &\,        & 3\,58\,30& 35\,10.5 &  A3V   &     10.20 &  0.61 &  0.86 &  0.56 &  0.28 &  0.17 &  0.34 &\,  2 \cr
172.\, & 31^\circ687 &\,   25239& 3\,58\,36& 32\,04.6 &  B9V   &      9.21 &  0.62 &  0.70 &  0.38 &  0.24 &  0.11 &  0.29 &\,  3 \cr
173.\, & 34^\circ791 &\,        & 3\,58\,42& 35\,14.3 &  K3III &      9.33 &  0.65 &  1.21 &  1.81 &  0.58 &  0.44 &  0.93 &\,  1 \cr
174.\, & 31^\circ689 &\,        & 3\,58\,50& 31\,52.3 &  A4:V   &      9.81 &  0.73 &  0.84 &  0.60 &  0.35 &  0.16 &  0.43 &\,  2 \cr
175.\, & 32^\circ708 &\,   25309& 3\,59\,25& 32\,46.3 &  B7V   &      8.46 &  0.49 &  0.53 &  0.31 &  0.20 &  0.09 &  0.26 &\,  2 \cr
176.\, & 34^\circ794 &\,   25308& 3\,59\,27& 35\,15.7 &  A0III &      8.52 &  0.82 &  0.83 &  0.40 &  0.27 &  0.15 &  0.34 &\,  2 \cr
177.\, & 32^\circ709 &\,         & 3\,59\,28& 32\,418 &  A3IV  &      9.81 &  0.80 &  0.91 &  0.51 &  0.24 &  0.15 &  0.33 &\,  2 \cr
178.\, & 31^\circ694 &\,         & 3\,59\,49& 31\,491 &  A1V   &      9.80 &  0.63 &  0.83 &  0.41 &  0.23 &  0.10 &  0.23 &\,  2 \cr
179.\, & 34^\circ801 &\,         & 4\,00\,25& 34\,416 &  B9V   &      9.70 &  0.61 &  0.77 &  0.36 &  0.22 &  0.11 &  0.26 &\,  2 \cr
180.\, & 32^\circ711 &\,         & 4\,01\,13& 32\,289 &  A8:V   &      9.66 &  0.64 &  0.80 &  0.62 &  0.30 &  0.16 &  0.39 &\,  3 \cr
181.\, & 33^\circ772 &\omit$\!\scriptstyle\rm $\hfil & 4\,01\,20& 33\,52.6 & A1V   &     10.49 &  0.71 &  0.89 &  0.46 &  0.24 &  0.15 &  0.30 &\,  2 \cr
182.\, & 33^\circ772 &\,         & 4\,01\,29& 33\,51.4 &  K3III-IV &   9.37 &  0.65 &  1.17 &  1.72 &  0.54 &  0.38 &  0.85 &\,  1 \cr
183.\, & 32^\circ714 &\,   25539& 4\,01\,32& 32\,26.1 &  B3V   &      6.81 &  0.26 &  0.33 &  0.23 &  0.17 &  0.07 &  0.19 &\,  2 \cr
184.\, & 32^\circ717 &\,         & 4\,02\,17& 32\,44.9 &  B9V   &      9.86 &  0.56 &  0.67 &  0.37 &  0.22 &  0.09 &  0.27 &\,  1 \cr
185.\, &             &\,         & 4\,02\,33& 32\,52.7 &  F9IV-V &    10.61 &  0.53 &  0.62 &  0.81 &  0.39 &  0.22 &  0.58 &\,  2 \cr
186.\!\!^*& 34^\circ809 &\,         & 4\,02\,42& 34\,29.7 &  A3V   &     10.24 &  0.60 &  0.84 &  0.52 &  0.25 &  0.13 &  0.32 &\,  2 \cr
187.\, & 33^\circ778 &\,         & 4\,02\,50& 34\,02.6 &  A1V   &     10.19 &  0.70 &  0.88 &  0.41 &  0.21 &  0.11 &  0.27 &\,  1 \cr
188.\!\!^*& 31^\circ703 &\,   25799& 4\,03\,28& 32\,15.1 &  B3V   &      6.97 &  0.27 &  0.35 &  0.25 &  0.18 &  0.08 &  0.21 &\,  2 \cr
189.\!\!^*& 33^\circ785 &\,   25833& 4\,03\,43& 33\,18.7 &  B3.5V &      6.92 &  0.28 &  0.39 &  0.23 &  0.16 &  0.08 &  0.18 &\,  2 \cr
\noalign{\vskip2mm\hrule\vskip2mm}
}}
\vfil\eject

\topinsert
{\rmn
\def\shift{
\hangindent=.9truecm\hangafter=1\noindent}
Notes
\vskip.2truecm
\shift
$\,$~~6. IDS 90-59 AB, $\Delta m$ = 1.6, $D$ = 2$.\!\!^{\prime\prime}$4 . Measured together.

\shift
~22. Photometric classification is uncertain. Possible photometric binary star 
as B3III+F5I.

\shift
~36. ADS 2696A, $\Delta m$ = 0.2, $D$ = 6$^{\prime\prime}$, measured separately.

\shift
~37. ADS 2696B.

\shift
~42. $V$ magnitude from Hoffleit (1982).

\shift
~63. ADS 2723, $\Delta m$ = 0.0, $D$ = 11.$\!\!^{\prime\prime}$4, measured separately.

\shift
~67. $o$ Per. $V$ magnitude from Hoffleit (1982).

\shift
~69. The star has considerably lower $Q_{XZS}$ values due to possible 
emission in the H$\alpha$ line.

\shift
~71. ADS 2729 AB, $\Delta m$ = 0.2, $D$ =1$^{\prime\prime}$. Measured together.

\shift
~77. ADS 2730, $\Delta m$ = 0.2, $D$ = 0.$\!\!^{\prime\prime}$45 . Measured together.

\shift
~97. LkH$\alpha$ 329 (Herbig and Rao 1972). The star has considerably 
lower $Q_{XZS}$ values.

\shift
102. LKH$\alpha$ 330 (Herbig and Rao 1972).

\shift
106. ADS 2723, $\Delta m$ = 0.0, $D$ = 11$^{\prime\prime}$. Measured together.

\shift
117. ADS 2771A.

\shift
118. ADS 2772AB, $\Delta m$ = 2.5, $D$ = 3$^{\prime\prime}$.

\shift
121. ADS 2784 AB, $\Delta m$ = 2.0, $D$ = 2$^{\prime\prime}$.

\shift
123. SB, Var V467 Per, eclipsing binary system.

\shift
127. ADS 2804 AB, $\Delta m$ = 4.7 , $D$ = 1$^{\prime\prime}$. Measured together.

\shift
147. ADS 2834 A, $\Delta m$ = 5.7, $D$ = 7$^{\prime\prime}$. Measured together. 

\shift
149. $V$ magnitude from Hoffleit (1982).

\shift
152. ADS 2857, $\Delta m$ = 2.3, $D$ = 3$^{\prime\prime}$. Measured together.

\shift
153. ADS 2859, $\Delta m$ = 5.8, $D$ = 22$^{\prime\prime}$. Var X Per, ($\gamma$ Cas type). Spectrum from Hoffleit (1982).

\shift
155. ADS 2866 AB, $\Delta m$ = 3.4, $D$ = 1$^{\prime\prime}$. Measured together.

\shift
159. Var, NSV 1418, $\beta$ Cep- type.

\shift
163. $V$ magnitude and spectrum from Hoffleit (1982).

\shift
186. ADS 2975 AB, $\Delta m$ = 0.2, $D$ = 2$^{\prime\prime}$. Measured together.

\shift
188. Var, NSV 1459, $V$ = 6.98 -- 7.27 (Hoffleit, 1982).

\shift
189. Var, AG Per, Eclipsing binary system. $\Delta m$ = 0.8, $D$ = 0.$\!\!^{\prime\prime}$8. 
Measured together.
}
\vskip-.5truecm
\endinsert

\topinsert
\Table{2}{ The results of photometric quantification of         
stars in the vicinity of the dark cloud L1470}
\vbox{\tabskip 33pt minus 33pt\baselineskip=10truept plus .1truept\rmn
\halign to \hsize{
\hfil$\scriptstyle#$&$\scriptstyle#$&$\scriptstyle\rm#$\hfil&
$\scriptstyle\rm#$\hfil&\hfil$\scriptstyle#$&\hfil$\scriptstyle#$&
\hfil$\scriptstyle#$&\hfil$\scriptstyle#$&\hfil$\scriptstyle#$\cr
\noalign{\vskip1mm\hrule\vskip1mm} 
\rm No.&\rm BD &\rm Sp* &\rm Sp\ (Viln) & V~ & M_V~ & E~ & A~ & r~\cr
\noalign{\vskip1mm\hrule\vskip1mm}
% No. BD        Sp.   Sp (Viln)   V     M   E    A     r
  4. & 30^\circ556 &       &  F2V    &   8.57 & +3.0 & 0.00 & 0.00 &  140 \cr   
  5. & 31^\circ622 &       &  K5III  &   9.83 & +0.6 & 0.39 & 1.47 &  356 \cr   
  7. & 30^\circ557 &       &  G9III  &   7.75 & +0.9 & 0.06 & 0.22 &  212 \cr   
  8. & 31^\circ624 &       &  F0V    &  10.86 & +3.0 & 0.23 & 0.80 &  258 \cr   
 10. & 30^\circ558 &       &  F5V    &   6.88 & +3.5 & 0.00 & 0.00 &   43 \cr   
 11. & 31^\circ625 &       &  A6V    &   9.36 & +2.4 & 0.23 & 0.78 &  172 \cr   
 12. &        &       &  F5V    &  11.13 & +3.6 & 0.19 & 0.65 &  238 \cr   
 13. & 30^\circ559 &       &  F7V    &  10.57 & +4.0 & 0.15 & 0.51 &  163 \cr   
 14. & 32^\circ649 &       &  F0V    &  10.21 & +2.8 & 0.19 & 0.65 &  225 \cr   
 15. & 31^\circ627 &       &  G2V    &  10.47 & +4.7 & 0.08 & 0.26 &  126 \cr   
 16. & 30^\circ560 & A5[2] &  A8V    &  10.08 & +2.8 & 0.14 & 0.49 &  228 \cr   
 17. &        &       &  G2V    &  11.49 & +4.5 & 0.13 & 0.43 &  205 \cr   
 18. &        &       &  F8V    &  11.24 & +4.1 & 0.17 & 0.56 &  207 \cr   
 19. & 32^\circ561 &       &  F0V    &   9.50 & +3.0 & 0.08 & 0.26 &  177 \cr   
 21. &        &       &  G2V    &  11.99 & +4.7 & 0.14 & 0.48 &  230 \cr   
 22. & 31^\circ629 & B5[2] & B3:III: &  9.10 & -2.5\rlap{:}& 1.43 & 4.75 & (294\rlap{\rms )} \cr   
 23. & 30^\circ561 & F0[2] &  F1V    &   9.88 & +3.1 & 0.13 & 0.43 &  186 \cr   
 24. & 30^\circ562 & F5[2] &  F7V    &  10.12 & +4.0 & 0.15 & 0.52 &  132 \cr   
 25. & 31^\circ630 &       &  K2V    &   8.79 & +7.0 & 0.00 & 0.00 &   23 \cr   
 26. &        &       &  G1V    &  11.14 & +4.5 & 0.27 & 0.95 &  137 \cr   
 27. &        &       &  F8III  &  12.33 & +1.0 & 0.56 & 1.93 &  758 \cr   
 28. & 31^\circ632 & A3[1] &  A9V    &   9.49 & +2.8 & 0.12 & 0.39 &  182 \cr   
 29. & 31^\circ633 &       &  G7V    &  10.21 & +5.5 & 0.00 & 0.00 &   87 \cr   
 30. & 30^\circ563 & F2[2] &  F7IV-V &   9.92 & +3.5 & 0.08 & 0.26 &  170 \cr   
 33. & 31^\circ634 &       &  A8V    &  10.14 & +2.8 & 0.13 & 0.44 &  240 \cr   
 34. & 31^\circ635 &       &  F7V    &  10.59 & +4.0 & 0.13 & 0.44 &  170 \cr   
 38. &        & A5[1] &  A4V    &  10.52 & +2.3 & 0.42 & 1.40 &  231 \cr   
 39. & 31^\circ637 &       &  F9V    &   9.00 & +4.0 & 0.02 & 0.05 &   96 \cr   
 40. &        &       &  G1V    &  12.10 & +4.5 & 0.28 & 0.96 &  213 \cr   
 41. & 30^\circ564 & F2[1] &  F2V    &   9.72 & +3.0 & 0.18 & 0.63 &  165 \cr   
 45. &        &       &  K3III &  12.64 & +0.6 & 0.56 & 2.11 &  968 \cr   
 47. & 32^\circ659 & F8[1] &  F4V    &   6.73 & +3.2 & 0.05 & 0.17 &   47 \cr   
 51. & 31^\circ639 &       &  K4V    &   9.10 & +7.0 & 0.00 & 0.00 &   26 \cr   
 54. &        &       &  G0V    &  11.97 & +4.4 & 0.34 & 1.15 &  192 \cr   
 57. & 32^\circ661 &       &  G0V    &   9.07 & +4.1 & 0.00 & 0.00 &  103 \cr   
 59. & 32^\circ662 &       &  F0V    &   9.27 & +2.9 & 0.16 & 0.54 &  140 \cr   
 65. &        &       &  K1IV-V &  13.10 & +5.0\rlap{:}& 0.38 & 1.37 & (222\rlap{\rms )} \cr   
 90. & 30^\circ568 & A3[1] &  A7IV   &   9.51 & +1.8 & 0.25 & 0.85 &  235 \cr   
 93. &        &       &  G5III  &  10.77 & +0.2 & 0.52 & 1.84 &  655 \cr   
110. & 32^\circ665 &       &  F2V    &   9.28 & +2.9 & 0.23 & 0.77 & 1132 \cr   
\noalign{\vskip1mm\hrule\vskip1mm} 
}
\hangindent.7truecm\hangafter=1
\noindent*~References for the spectra: [1] Cannon and Mayall (1949), [2]  AGK 3 catalog.

}
\vskip-.4truecm plus.2truecm
\endinsert


\topinsert
\Table{3}{ Distances of the Perseus dark clouds}
\vbox{\tabskip 33pt minus 33pt\rmn
\halign to \hsize{
# \hfil&& # \hfil\cr
\noalign{\vskip2mm\hrule\vskip2mm}
Source & Distance~(pc) & Method\cr
\noalign{\vskip2mm\hrule\vskip2mm}
Heeschen (1951)        & 200-300, 800   &   star counts             \cr
Lynds (1969)           & 200-300        &   galaxy counts           \cr
Cernicharo et al. (1985) & 200, 300      &    star counts            \cr
\v Cernis (1990)       &    160 and 220 &      photometric distance \cr      
This work              & 160 and 260    &   photometric distance    \cr 
\noalign{\vskip2mm\hrule\vskip2mm}
}}
\endinsert

\pageinsert
\Table{4}{ The results of photometric quantification of IC~348 stars}
\vbox{\tabskip 33pt minus 33pt\baselineskip=9.6truept\rmn
\halign to \hsize{
\hfil$\scriptstyle#$&$\scriptstyle#$&
\hfil$\scriptstyle\rm#$&\hfil$\scriptstyle\rm#$&
$\scriptstyle\rm#$\hfil&$\scriptstyle\rm#$\hfil&
\hfil$\scriptstyle#$&\hfil$\scriptstyle#$&\hfil$\scriptstyle#$\hfil&
\hfil$\scriptstyle#$&\hfil$\scriptstyle#$&\hfil$\scriptstyle\rm#$\cr
\noalign{\vskip1mm\hrule\vskip1mm}
\rm No.&\rm BD &\rm G &\rm F &\rm Sp* &\rm Sp\ (Viln) & V~ & M_V~ & E_{B-V}~ & A_V~ & r~ & Mem \cr
\noalign{\vskip1mm\hrule\vskip1mm}
 %No.        BD        G      F       Sp.         Sp(Viln)       V         M       E        A         r      Mb      
 35. &     31^\circ636  &     &   1M  &  G0[5]    &    G2V      &    9.98 &   +4.7  &  0.00  &  0.00 &    115  &  nm   \cr  
 43. &             &     &       &           &    K3.5V    &   12.67 &   +6.9  &  0.08  &  0.30 &    118  &  nm   \cr  
 44. &     31^\circ638  &     &    1  &           &    G1V      &    9.66 &   +4.7  &  0.00  &  0.00 &    100  &  nm   \cr  
 46. &             &     &       &           &    A6IV     &   12.40 &   +1.9  &  0.78  &  2.64 &    372  &   m\rlap{\rms ?}  \cr  
 48. &             &     &    2  &           &    K2V      &   11.05 &   +6.5  &  0.00  &  0.00 &     81  &  nm   \cr  
 49. &             &     &    3  &           &    G1V      &   12.46 &   +4.7  &  0.14  &  0.48 &    286  &  nm\rlap{\rms ?}  \cr  
 52. &     31^\circ640  &     &    4  &           &    A3V      &   11.40 &   +1.5  &  0.90  &  3.03 &    236  &   m   \cr  
 56. &             &   1 &    5  &  G8-K0[4] &    K0III    &   12.76 &   +0.8  &  0.46  &  1.66 &   1159  &  nm   \cr  
 58. &             &   2 &    6  &  F8-G0[4] &    G2IV     &   12.75 &   +3.0  &  0.46  &  1.59 &   (429\rlap{\rms )} &   m\rlap{\rms ?}  \cr  
 62. &             &   3 &    7  &  F8[5]    &    F9.5V    &   11.34 &   +4.3  &  0.16  &  0.55 &    198  &  nm   \cr  
 63.\rlap{*} &     31^\circ641  &   4 &    8  &  A0V[3]   &    A3V      &    9.89 &   +1.9  &  0.36  &  1.20 &    238  &   m   \cr  
 64.\rlap{*} &            &   5 &    9  &  A2V[3]   &    A3V      &   10.00 &   +1.9  &  0.39  &  1.31 &    226  &   m   \cr  
 66.\rlap{*} &            &   6 &   10  &  F0III,V[3] &   F2V      &   11.91 &   +3.2  &  0.40  &  1.37 &    290  &   m   \cr  
 67. &     31^\circ642  &     &       &  B1III[3] &    B1III    &    3.83 &   -4.4  &  0.29  &  0.96 &    284  &   m   \cr  
 68. &             &   7 &   11  &  F8[5]    &    G0V      &   11.62 &   +4.4  &  0.17  &  0.60 &    212  &  nm   \cr  
 69. &             &   8 &   12  &  F8[4]    &    F9Ve?    &   13.47 &   +4.3  &  0.65  &  2.25 &    242  &   m   \cr  
 70.\rlap{*} &            &   9 &   13  &  F2IV,V[3] &   F1:IV    &   11.55 &   +2.3  &  0.65  &  2.21 &    256  &   m   \cr  
 72. &             &     &       &           &    A1V      &   11.68 &   +1.7  &  0.85  &  2.86 &    265  &   m   \cr  
 73.\rlap{*} &            &  10 &   14  &  A2V[3]   &    A4V      &   11.75 &   +2.1  &  0.69  &  2.34 &    290  &   m   \cr  
 74.\rlap{*} &            &  11 &   15  &  F0m:[3]  &    A8III-IV &   10.60 &   +1.3  &  0.70  &  2.38 &    243  &   m   \cr  
 75. &             &     &       &           &    G3:Ve?   &   13.92 &   +4.8  &  0.65  &  2.27 &    234  &   m   \cr  
 76. &             &     &   16  &           &    F8:Ve?   &   13.34 &   +4.0\rlap{:}  &  0.80  &  2.73 &   (210\rlap{\rms )}  &   m   \cr  
 77.\rlap{*} &    31^\circ643  &     &   17  &  B5V[3]   &    B4.5V    &    8.52 &   -0.3  &  0.80  &  2.66 &    236  &   m   \cr  
 78.\rlap{*} &            &  12 &   18  &  A2III[3] &    A3IV     &   10.21 &   +0.8  &  0.77  &  2.60 &    230  &   m   \cr  
 79.\rlap{*} &            &  13 &   19  &  F8[4]    &    G7IVe?   &   12.94 &   +3.0  &  0.84  &  2.99 &    245  &   m   \cr  
 80. &             &     &       &           &    B8V      &   14.02 &   +1.0  &  1.68  &  5.63 &    305  &   m   \cr  
 81. &             &     &       &           &    G1V      &   13.77 &   +4.6  &  0.57  &  1.99 &    273  &   m   \cr  
 82. &             &     &       &           &    K5III    &   12.74 &   +0.3  &  0.77  &  2.82 &    839  &  nm   \cr  
 83. &             &  14 &       &           &    K5:Ve?   &   13.95 &   +6.5\rlap{:} &  0.17  &  0.64 &   (230\rlap{\rms )}  &   m   \cr  
 84. &             &  15 &       &           &    K3V      &   13.25 &   +6.5\rlap{:} &  0.16  &  0.56 &   (173\rlap{\rms )} &   m\rlap{\rms ?}  \cr  
 85. &             &  16 &       &  A0[4]    &    B5V      &   11.23 &   +0.1  &  1.17  &  4.13 &    275  &   m   \cr  
 86. &             &     &       &           &    K2III    &   12.81 &   +0.7  &  0.91  &  3.37 &    560  &  nm   \cr  
 87. &             &     &       &           &    A7V      &   13.32 &   +2.6  &  1.06  &  3.62 &    263  &   m   \cr  
 89. &             &  17 &   20  &  G1III[4] &    G0IVe?   &   12.65 &   +3.0  &  0.61  &  2.11 &    322  &   m   \cr  
 91. &             &     &       &           &    K3III    &   13.34 &   +0.6  &  0.79  &  2.97 &    899  &  nm   \cr  
 92. &             &  18 &       &  K2[4]    &    K0V:     &   13.09 &   +5.0\rlap{:} &  0.37  &  1.24 &   (234\rlap{\rms )} &   m\rlap{\rms ?}  \cr  
 94. &             &     &   21  &  G0[5]    &    F6V      &   11.63 &   +4.0  &  0.23  &  0.77 &    236  &   m   \cr  
 95. &             &     &       &           &    A7m:     &   11.72 &   +1.7  &  0.90  &  3.07 &    245  &   m   \cr  
 96. &     31^\circ644  &  19 &   22  &  K0[3]    &    G9III-IV &    7.87 &   +1.6  &  0.25  &  0.89 &    119  &  nm   \cr  
 97. &             &     &       &  ..e[6]   &    K5IV-Ve  &   14.63 &   +5.0\rlap{:} &  0.64  &  2.30 &    292  &   m   \cr  
 98. &             &     &   23  &           &    G2IV-V   &   11.97 &   +4.7  &  0.16  &  0.56 &    220  &  nm   \cr  
 99.\rlap{*} &    31^\circ645  &     &   24  &  B5[5]    &    B3V      &    9.13 &   +1.0  &  0.89  &  3.13 &    251  &   m   \cr  
102. &             &     &   25  &  G2e[6]   &    F9IVe    &   12.10 &   +2.5  &  0.73  &  2.51 &    261  &   m   \cr  
103. &             &     &   26  &  A[5]     &    A2V      &   11.88 &   +1.8  &  0.77  &  2.58 &    316  &   m\rlap{\rms ?}  \cr  
104. &             &     &   27  &           &    G2V      &   12.01 &   +4.7  &  0.26  &  0.91 &    191  &  nm   \cr  
105. &             &     &   28  &           &    G5IV-V   &   11.37 &   +4.0  &  0.27  &  0.95 &    191  &  nm   \cr  
\noalign{\vskip1mm\hrule\vskip1mm}
}
\vfill
\hangindent.7truecm\hangafter=1
\noindent*~{\bfn Remarks:} Numbers of the most reliable cluster members, 
estimated by Fredrick (1956), are marked by asterisks. References for spectra:
[3] Harris et al. (1954), [4] Strom et al. (1974), [5] Vyssotsky
and Williams (1948), [6] Herbig and Rao (1972).}
\vfil\endinsert

\pageinsert
\Table{5}{ Distance of the open cluster IC~348}
\vbox{\tabskip 33pt minus 33pt\rmn
\halign to \hsize{
# \hfil& \hfil#\hfil & # \hfil\cr
\noalign{\vskip1mm\hrule\vskip1mm}
Source & Distance~(pc) & Method\cr
\noalign{\vskip1mm\hrule\vskip1mm}
Gingrich (1922)       &     107    &           proper motion study         \cr
Greenstein (1948)     &     160    &           spectroscopic parallaxes    \cr
Harris et al. (1954)  &     380    &           spectroscopic parallaxes    \cr
Fredrick (1956)       &     480    &           proper motion study         \cr 
Strom et al. (1974)   &     330    &           spectroscopic parallaxes    \cr 
This work             &     260    &           photometric distance        \cr
\noalign{\vskip1mm\hrule}
}}
\vfil\endinsert


\pageinsert
\Table{6}{  The results of photometric quantification of stars in the
region of the association Per OB2.}
\vbox{\tabskip 33pt minus 33pt\baselineskip=9.9truept\rmn
\halign to \hsize{
\hfil$\scriptstyle#$&$\scriptstyle#$&$\scriptstyle\rm#$\hfil&
$\scriptstyle\rm#$\hfil&\hfil$\scriptstyle#$&\hfil$\scriptstyle#$&
\hfil$\scriptstyle#$\hfil&\hfil$\scriptstyle#$&\hfil$\scriptstyle#$
&\hfil$\scriptstyle\rm#$\cr
\noalign{\vskip1mm\hrule\vskip1mm} 
\rm No.&\rm BD &\rm Sp* &\rm Sp\ (Viln) & V~ & M_V~ & E_{B-V}~ & A_V~ & r~ & Mem \cr
\noalign{\vskip1mm\hrule\vskip1mm}
% No.   BD   Sp(MK)  Sp(Viln.)   V     M    E    A    r  Mem.
  1. &  37^\circ779 &            & F3V      &   9.29  & +3.3  & 0.06  & 0.22   & 143   &         \cr  
  2. &  37^\circ794 &  B9III[7]  & B7III    &   7.57  & -1.0  & 0.22  & 0.75   & 366   & OB      \cr  
  3. &  37^\circ796 &  A1V[7]    & A1V      &   9.83  & +1.1  & 0.29  & 0.98   & 355   & OB      \cr  
  6. &  36^\circ730 &  A1V[7]    & A0V      &  10.50  & +1.6  & 0.38  & 1.27   & 336   & OB      \cr  
  9. &  36^\circ731 &  B9V[7]    & B8.5V    &   9.58  & +0.3  & 0.42  & 1.40   & 377   & OB      \cr  
 20. &  37^\circ808 &  A4IV[7]   & A4:IV    &   9.70  & +1.2  & 0.46  & 1.53   & 248   & OB      \cr  
 31. &  34^\circ712 &            & K1III    &   7.81  & +0.8  & 0.07  & 0.26   & 224   &         \cr  
 32. &  37^\circ814 &  A1V[7]    & A0V      &   7.74  & +0.8  & 0.11  & 0.39   & 204   & OB      \cr  
 36. &  36^\circ735 &  B9.5II[7] & B8.5IV   &   9.89  & +0.0  & 0.43  & 1.45   & 488   & OB      \cr  
 37. &  36^\circ735 &  G8V:[7]   & G8III-IV &  10.12  & +2.0  & 0.34  & 1.20   & 242   & OB      \cr  
 42. &  33^\circ698 &  B1IV[8]   & B1V      &   4.97  & +3.3  & 0.27  & 0.89   & 292   & OB      \cr  
 50. &  32^\circ660 &            & A5V      &   9.25  & +2.3  & 0.31  & 1.05   & 151   &         \cr  
 53. &  33^\circ703 &            & A1V      &  10.82  & +1.7  & 0.55  & 1.83   & 287   &         \cr  
 55. &  33^\circ704 &  B2IV-V[7] & B3V      &   7.44  & +1.7  & 0.29  & 0.97   & 431   & OB      \cr  
 60. &  33^\circ706 &  B7V[7]    & B8V      &  10.16  & +1.0  & 0.33  & 1.10   & 409   & OB      \cr  
 61. &  36^\circ741 &  A5V[7]    & A2V      &   8.85  & +1.3  & 0.12  & 0.39   & 270   & OB      \cr
 71. &  35^\circ744 &  A2IV[7]   & A1V      &   8.32  & +1.1  & 0.21  & 0.72   & 273   & OB      \cr  
 88. &  30^\circ567 &            & A0IV     &   9.88  & +0.2  & 0.53  & 1.78   & 380   &         \cr  
100. &  33^\circ712 &  A7III[7]  & A4V      &  10.30  & +2.1  & 0.46  & 1.57   & 211   & OB      \cr  
107. &  33^\circ714 &  A4V[7]    & A4V      &  10.38  & +2.1  & 0.29  & 0.96   & 291   & OB      \cr  
108. &  37^\circ827 &  A0[8]     & A1V      &  11.32  & +1.7  & 0.40  & 1.32   & 457   & OB      \cr  
111. &  37^\circ828 &  Am[7]     & A5IV:    &   9.37  & +1.4  & 0.55  & 1.87   & (166\rlap{\rms )} & OB\rlap{\rms ?} \cr  
112. &  34^\circ730 &            & F2V      &  10.30  & +3.1  & 0.13  & 0.43   & 226   &         \cr  
113. &  34^\circ730 &            & K5III:   &  10.31  & +3.0\rlap{:} & 0.12  & 0.45   & (236\rlap{\rms )} &         \cr  
114. &  32^\circ666 &  A0III[7]  & B9.5III  &   9.72  & -0.4  & 0.38  & 1.27   & 589   & (OB\rlap{\rms )}     \cr  
115. &              &            & F8V      &  11.00  & +4.1  & 0.28  & 0.96   & 154   &         \cr  
116. &              &            & F5V      &  11.11  & +3.6  & 0.14  & 0.48   & 255   &         \cr  
117. &  34^\circ732 &  A0V[7]    & B8.5V    &   9.53  & +0.6  & 0.28  & 0.92   & 400   & OB      \cr  
118. &  33^\circ717 &  B2.5V[8]  & B2V      &   6.53  & -2.5  & 0.35  & 1.14   & 378   & OB      \cr  
119. &  31^\circ652 &            & A8V      &   8.15  & +2.4  & 0.21  & 0.70   & 102   & OB\rlap{\rms ?} \cr  
120. &  31^\circ653 &  A3V[7]    & A2.5IV   &  10.39  & +1.0  & 0.41  & 1.40   & 396   & OB      \cr  
121. &  31^\circ655 &  B5Vn[7]   & B6V      &   7.40  & +0.5  & 0.28  & 0.92   & 248   & OB      \cr  
122. &  34^\circ739 &  B8V[7]    & B7V      &   8.47  & +0.1  & 0.23  & 0.77   & 331   & OB      \cr  
123. &  32^\circ667 &  A3[9]     & A2V      &   5.14  & +1.8  & 0.07  & 0.23   & (58\rlap{\rms )}  & OB\rlap{\rms ?} \cr  
124. &  31^\circ657 &  A0V[7]    & B9V      &   9.48  & +1.0  & 0.22  & 0.74   & 353   & OB      \cr  
125. &  31^\circ658 &            & B6V      &   8.52  & +0.3  & 0.41  & 1.36   & 236   & OB      \cr  
126. &  31^\circ659 &  A3IV[7]   & A4.5IV   &   9.23  & +1.4  & 0.31  & 1.03   & 229   & OB      \cr
127. &  32^\circ669 &  A7V[7]    & A6V      &   9.04  & +2.2  & 0.26  & 0.87   & 156   &(OB\rlap{\rms )}       \cr  
128. &  36^\circ763 &  A9V[7]    & A8V      &   9.07  & +2.6  & 0.14  & 0.48   & 158   &(OB\rlap{\rms )}       \cr  
129. &  34^\circ748 &  A0V[7]    & B9.5V    &   9.73  & +1.1  & 0.24  & 0.81   & 366   & OB      \cr  
130. &  34^\circ753 &  B9V[7]    & B8V      &   9.20  & +0.1  & 0.29  & 0.97   & 423   & OB      \cr
131. &  33^\circ727 &            & K1III    &   9.67  & -0.5  & 0.00  & 0.00   &1081   &         \cr
132. &  33^\circ728 &  B0.5V[8]  & B1V      &   5.75  & -3.2  & 0.29  & 0.97   & 394   & OB      \cr
133. &  30^\circ581 &            & A0V      &  10.89  & +1.6  & 0.41  & 1.37   & 384   &         \cr
134. &  30^\circ582 &            & A5V      &   6.18  & +2.1  & 0.04  & 0.13   &  62   &         \cr
135. &  32^\circ674 &  A0II[7]   & A5I-II   &   8.92  & -4.1  & 0.42  & 1.43   &2080   &         \cr
136. &  33^\circ730 &  B2Vn[8]   & B2V      &   7.41  & -2.5  & 0.31  & 1.03   & 597   &(OB\rlap{\rms )}        \cr
137. &  34^\circ755 &  A0p(Si)[7]& B9.5V    &   9.58  & +0.8  & 0.20  & 0.66   & 421   & OB      \cr
138. &  30^\circ584 &            & A6V      &   9.64  & +2.2  & 0.38  & 1.27   & 175   &         \cr
139. &  32^\circ676 &  A0V[7]    & A0V      &   9.71  & +0.8  & 0.28  & 0.92   & 396   & OB      \cr
}}
\vfil
\endinsert
\pageinsert
\null\vfill
\line{\hfil\rml Table~6~(continued)~~~}
\vbox{\tabskip 33pt minus 33pt\baselineskip=9.9truept\rmn
\halign to \hsize{
\hfil$\scriptstyle#$&$\scriptstyle#$&$\scriptstyle\rm#$\hfil&
$\scriptstyle\rm#$\hfil&\hfil$\scriptstyle#$&\hfil$\scriptstyle#$&
\hfil$\scriptstyle#$\hfil&\hfil$\scriptstyle#$&\hfil$\scriptstyle#$
&\hfil$\scriptstyle\rm#$\cr
\noalign{\vskip1mm\hrule\vskip1mm} 
\rm No.&\rm BD &\rm Sp* &\rm Sp\ (Viln) & V~ & M_V~ & E_{B-V}~ & A_V~ & r~ & Mem \cr
\noalign{\vskip1mm\hrule\vskip1mm}
140. &  35^\circ757 &  Am[7]     & A4V      &  10.09  & +1.7  & 0.27  & 0.91   & 313   & OB      \cr
141. &  31^\circ662 &            & G7III    &   6.70  & +1.8  & 0.04  & 0.13   &  90   &         \cr
142. &  34^\circ758 &  A2V[7]    & A1V      &   9.48  & +1.7  & 0.18  & 0.59   & 274   & OB      \cr
143. &  36^\circ769 &  A0V[7]    & B9.5V    &   9.75  & +0.6  & 0.37  & 1.23   & 383   & OB      \cr
144. &  34^\circ759 &  A8III[7]  & A7IV     &  10.18  & +1.7  & 0.23  & 0.78   & 347   & OB      \cr
145. &  35^\circ763 &  B6V[7]    & B5.5V    &   8.65  & -0.1  & 0.23  & 0.75   & 398   & OB      \cr
146. &  35^\circ764 &  B9.5V[7]  & B7V      &   9.42  & +0.4  & 0.27  & 0.90   & 421   & OB      \cr
147. &  34^\circ761 &  B8V[7]    & B7V      &   8.80  & +0.6  & 0.24  & 0.81   & 301   & OB      \cr
148. &  32^\circ679 &  A5III[7]  & A3V      &   8.26  & +1.5  & 0.22  & 0.68   & 164   &(OB\rlap{\rms )}       \cr
149. &  31^\circ666 &  B1Ib[8]   & B1Ib     &   2.85  & +5.9  & 0.32  & 1.06   & 345   & OB      \cr
150. &  32^\circ683 &  A5IV[7]   & A2V      &   8.96  & +1.3  & 0.27  & 0.92   & 223   & OB      \cr
151. &  30^\circ589 &            & A2V      &   9.49  & +1.7  & 0.51  & 1.70   & 167   &         \cr
152. &  34^\circ766 &  A1V[7]    & A1V      &   9.52  & +1.7  & 0.28  & 0.94   & 238   & OB      \cr
153. &  30^\circ591 &  O9.5p[8]  & O9.5ep   &   6.10  & +4.2  & 0.60  & 1.99   & 459   & OB      \cr
154. &  34^\circ767 &  B7V[7]    & B7V      &   8.96  & +0.1  & 0.23  & 0.77   & 415   & OB      \cr
155. &  31^\circ669 &  B8V[7]    & B8V      &   8.60  & +0.5  & 0.30  & 1.01   & 262   & OB      \cr
156. &  33^\circ741 &  A0V[7]    & A0V      &   9.98  & +1.5  & 0.21  & 0.70   & 353   & OB      \cr
157. &  31^\circ670 &  B8V[7]    & B9.5V    &   8.87  & +1.2  & 0.30  & 1.00   & 216   & OB      \cr
158. &  33^\circ743 &  A8IV[7]   & A7IV:    &   9.53  & +1.7  & 0.27  & 0.92   & 241   & OB      \cr
159. &  34^\circ768 &  B1.5V[8]  & B1V      &   5.46  & -3.3  & 0.27  & 0.88   & 374   & OB      \cr
160. &  35^\circ771 &            & F8V      &   8.29  & +4.0  & 0.03  & 0.09   &  69   &         \cr
161. &  32^\circ691 &  A0IV[7]   & B9V      &   8.55  & +0.5  & 0.25  & 0.83   & 278   & OB      \cr
162. &  35^\circ772 &            & K3III    &   9.03  & +0.6  & 0.21  & 0.80   & 336   &         \cr
163. &  35^\circ775 &  O8III[8]  & O8III    &   4.02  & -5.6  & 0.35  & 1.14   & 497   & OB      \cr
164. &  32^\circ697 &  A0V[7]    & A1V      &   8.36  & +1.5  & 0.27  & 0.91   & 168   &(OB\rlap{\rms )}       \cr
165. &  32^\circ698 &  A8(Sr)[7] & A7:IV    &   9.85  & +1.9  & 0.27  & 0.92   & 255   & OB      \cr
166. &  31^\circ680 &  B6V[7]    & B6V      &   9.31  & +0.3  & 0.26  & 0.88   & 423   & OB      \cr
167. &  35^\circ781 &  A1V[7]    & A1V      &   9.90  & +1.7  & 0.29  & 0.98   & 278   & OB      \cr
168. &  32^\circ703 &  B9V[7]    & B8.5V    &   8.53  & +1.2  & 0.21  & 0.70   & 212   & OB      \cr
169. &  34^\circ788 &            & F5V      &  10.28  & +3.6  & 0.17  & 0.57   & 167   &         \cr
170. &  31^\circ686 &  A1V[7]    & A3V      &   8.86  & +1.7  & 0.23  & 0.76   & 191   &(OB\rlap{\rms )}      \cr
171. &  34^\circ790 &  Am[7]     & A3V      &  10.20  & +1.5  & 0.29  & 0.98   & 350   & OB      \cr
172. &  31^\circ687 &  B9.5V[7]  & B9V      &   9.21  & +0.3  & 0.28  & 0.92   & 396   & OB      \cr
173. &  34^\circ791 &            & K3III    &   9.33  & +0.6  & 0.17  & 0.63   & 419   &         \cr
174. &  31^\circ689 &  A0III[7]  & A4:V     &   9.81  & +1.9  & 0.33  & 1.11   & 229   & OB      \cr
175. &  32^\circ708 &  B6V[7]    & B7V      &   8.46  & +0.3  & 0.24  & 0.79   & 393   & OB      \cr
176. &  34^\circ794 &  A0IV[7]   & A0III    &   8.52  & -0.1  & 0.31  & 1.03   & 330   & OB      \cr
177. &  32^\circ709 &  A3V[7]    & A3IV     &   9.81  & +1.0  & 0.24  & 0.81   & 398   & OB      \cr
178. &  31^\circ694 &  A0V[7]    & A1V      &   9.80  & +1.6  & 0.19  & 0.62   & 328   & OB      \cr
179. &  34^\circ801 &  A0V[7]    & B9V      &   9.70  & +0.9  & 0.25  & 0.83   & 393   & OB      \cr
180. &  32^\circ711 &  Am[7]     & A8:V     &   9.66  & +2.3  & 0.21  & 0.70   & 215   & OB      \cr
181. &  33^\circ772 &   A1[9]    & A1V      &  10.49  & +1.7  & 0.28  & 0.93   & 373   & OB      \cr
182. &  33^\circ772 &            & K3III-IV &   9.37  & +4.0\rlap{:} & 0.07  & 0.26   & (264\rlap{\rms )} &         \cr
183. &  32^\circ714 &  B3V[8]    & B3V      &   6.81  & +1.3  & 0.24  & 0.79   & 288   & OB      \cr
184. &  32^\circ717 &  B95II[7]  & B9V      &   9.86  & +0.9  & 0.22  & 0.74   & 441   & OB      \cr
185. &              &            & F9IV-V   &  10.61  & +3.4  & 0.13  & 0.43   & 227   &         \cr
186. &  34^\circ809 &  A7V[7]    & A3V      &  10.24  & +1.9  & 0.21  & 0.70   & 337   & OB      \cr
187. &  33^\circ778 &  A2V[7]    & A1V      &  10.19  & +1.4  & 0.19  & 0.63   & 429   & OB      \cr
188. &  31^\circ703 &  B3V[8]    & B3V      &   6.97  & +1.7  & 0.27  & 0.88   & 361   & OB      \cr
189. &  33^\circ785 &  B5pV[8]   & B3.5V    &   6.92  & -1.5  & 0.21  & 0.70   & 350   & OB      \cr
\noalign{\vskip1mm\hrule}
}}
\vfil
\endinsert

\topinsert
\Table{7}{ Distance of the Per~OB2 association}
\vbox{\tabskip 33pt minus 33pt\rmn
\halign to \hsize{
# \hfil& \hfil#\hfil & # \hfil\cr
\noalign{\vskip1mm\hrule\vskip1mm}
Source & Distance~(pc) & Method\cr
\noalign{\vskip2mm\hrule\vskip2mm}
Blaauw (1952)               & 300  &     spectroscopic parallaxes     \cr
Morgan et al. (1953)         & 360  &     spectroscopic parallaxes     \cr
Seyfert et al. (1960)        & 400  &     spectroscopic parallaxes     \cr
Borgman and Blaauw (1964)   & 334  &     photometric distance         \cr
Racine (1968)               & 330  &     spectroscopic parallaxes     \cr
Guetter (1977)              & 413  &     spectroscopic parallaxes     \cr
Klochkova and Kopylov (1985) & 340 &     spectroscopic parallaxes     \cr
This work                   & 338  &     photometric distance         \cr
\noalign{\vskip1mm\hrule\vskip1mm}
}}
\endinsert
\bye%
