#Table: J/A+A/417/263/notes.dat (http://cdsarc.cds.unistra.fr)
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Name     |Text
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TW And   |HIP d=232(67) pc, periodic variable; magnetic activity and evolution
TW And   | (And_12); status of evolution (And_7); radio emission (And_13).
UU And   |Period jumps (And_2).
WW And   |Accretion disk (And_14); radio emission (And_15, And_16).
XZ And   |Period change (And_17, And_18, And_4); radio emission (And_15).
AA And   |Periodic variable (HIP).
DW Aps   |HIP d=490(280) pc, periodic variable; radio emission (Aps_1).
RY Aqr   |Different absolute parameters (B&D); magnetic activity and evolution
RY Aqr   | (Aqr_3, Aqr_4); radio emission (Aqr_5).
CZ Aqr   |Period change (Aqr_6).
XZ Aql   |Period change (Aql_1).
YZ Aql   |Extrasolar planet (Aql_10).
FK Aql   |Period change (Aql_11).
KO Aql   |HIP d=265(75) pc, periodic variable; radio emission (Aql_12, Aql_13);
KO Aql   | mass transfer (Aql_14).
QY Aql   |Extrasolar planet (Aql_10); radio emission (Aql_13).
V342 Aql |Duplicity-induced variability (HIP); mass flow (Aql_15); accretion
V342 Aql | disks (Aql_16).
V346 Aql |Mass transfer (Aql_14); radio emission (Aql_12).
R Ara    |HIP d=80+/-13pc and multiple system; d=166.7 pc and X-ray emission
R Ara    | (Ara_5); radio emission (Ara_6).
RW Ara   |Radio emission (Ara_6); mass transfer (Ara_7).
SX Aur   |HIP d=320(140) pc and periodic variable; d=1200(200) pc (Aur_3);
SX Aur   | different absolute parameters (Aur_1); reversals of mass transfer
SX Aur   | (Aur_8).
AK Aur   |Visual companion (Aur_9).
AM Aur   |Radio continuum emission (Aur_10; Aur_11; Aur_12).
IM Aur   |d=359 pc (Aur_4); d=434.8 pc (Aur_7); complex period variations
IM Aur   | (Aur_13); H? mass transfer structures (Aur_14); apsidal motion
IM Aur   | (Aur_15; Aur_16); radio emission (Aur_17); X-ray emission (Aur_7).
Y Cam    |HIP periodic variable; pulsating component in the system (Cam_4);
Y Cam    | possibly 4-body system (Cam_5).
SS Cam   |HIP d=320(180) pc, periodic variable, new classified; X-ray
SS Cam   | variability (Cam_7).
S Cnc    |HIP d=340(130) pc and periodic variable; radio emission (Cnc_3);
S Cnc    | X-ray emission (Cnc_4).
RY Cnc   |Probably periodic variable (KKN).
RZ Cnc   |HIP d=310(150)pc and periodic variable; circumstellar matter (Cnc_7);
RZ Cnc   | chromospherically active binary (Cnc_8).
RU Cnc   |HIP d=330(170) pc and periodic variable; differential rotation and
RU Cnc   | activity cycle (Cnc_9); only photoelectric observations
RU Cnc   | (Cnc_10, Cnc_11).
TU Cnc   |Possible mass and angular momentum loss (Cnc_12).
R CMa    |Third body (CMa_10).
AK CMi   |Period change (CMi_1).
RX Cas   |HIP  d=330(190) pc; W-Ser type (Cas_22);
RX Cas   | Very fast mass transfer (Cs_3).
RZ Cas   |HIP d=62.5(2.4) pc; Frequent unpredictable period variations (Cas_4);
RZ Cas   | A possible thirdbody (Cas_5). Third body or apsidal motion (Cas_17).
RZ Cas   | Low level of magnetic activity (Cas_17).
SX Cas   |Third body (Cas_19); System, enduring slow mass transfer (Cas_24).
TV Cas   |HIP d=254(49) pc; Period variation (Cas_20).
AB Cas   |HIP d=300(120) pc; Eclipsing binary with pulsating components
AB Cas   | (Cas_25, Cas_26), Mass transfer and third body from O-C analysis
AB Cas   | (Cep_27).
DO Cas   |HIP d=147(21) pc.
CT Cen   |TYC d=56(49) pc.
V379 Cen |HIP d=231(72) pc.
U Cep    |HIP d=207(23) pc; Disk structure (Cep_20); Variable mass transfer
U Cep    | activity (Cep_21), Complex orbital period variation (Cep_1, KKN).
RS Cep   |Circumstellar matter (Cep_16); Orbital period variation (Cep_22, KKN)
XX Cep   |HIP d=314(93) pc; Third body (Cep_23), Orbital period variation (KKN)
XY Cep   |HIP d=340(140) pc, Orbital period variation (KKN).
EK Cep   |HIP d=153(14) pc; Apsidal motion and the secondary component seems to
EK Cep   | be in the pre-main sequence phase (Cep_24, KKN).
AT Cir   |HIP d=168(25) pc and periodic variable.
RW CrA   |HIP periodic variable.
V681 CrA |HIP d= 219(45) pc.
U CrB    |HIP d=338(95) pc, periodic variable; third body (CrB_1); UPS
U CrB    | photoelectric observations (CrB_2).
RW CrB   |HIP d= 196(63) pc, periodic variable; possible mass and angular
RW CrB   | momentum loss (CrB_6).
SW Cyg   |Period jumps (Cyg_33); period changes (Cyg_34, Cyg_35, Cyg_36);
SW Cyg   | accretion disk (Cyg_37).
SY Cyg   |Apsidal motion (Cyg_29).
UW Cyg   |TYCHO d=20 pc.
VW Cyg   |HIP d=610 pc.
WW Cyg   |HIP d=740 pc;  period change (Cyg_38); accretion disk (Cyg_39).
ZZ Cyg   |Delta Scuti type physical  variability of the hotter component
ZZ Cyg   | (Cyg_40).
CG Cyg   |RSCVn, period change (Cyg_41, Cyg_42, Cyg_43).
KU Cyg   |Accretion disk (Cyg_44, Cyg_16, Cyg_45, Cyg_46).
MY Cyg   |Displeced secondary minimum (Cyg_25).
V463 Cyg |Displeced secondary minimum (Cyg_25) third light (Cyg_17).
V512 Cyg |Displeced secondary minimum (Cyg_25).
V753 Cyg |Accretion disk (Cyg_39).
V909 Cyg |Triple star (Cyg_47).
V959 Cyg |Displeced secondary minimum (Cyg_25).
V1898 Cyg|HIP d=620 pc.
V2080 Cyg|HIP d=79.4 pc.
W Del    |Accretion disk (Del_10); apsidal motion (Del_9).
TT Del   |Period change (Del_11).
FZ Del   |Period change (Del_12); eccentric orbit (Del_13).
Z Dra    |HIP d=236 pc.
RR Dra   |Period change, period jumps (Dra_20); accretion disk (Dra_21).
RZ Dra   |HIP d=550 pc; third body, period change (Dra_8).
TW Dra   |HIP d=122 pc; third body, period change (Dra_22); accretion disk
TW Dra   |(Dra_21).
AI Dra   |HIP d=142 pc; period change, third body (Dra_10) accretion disk
AI Dra   | (Dra_21).
BF Dra   |HIP d=560 pc; system with eccentric orbit (Dra_6).
S Equ    |HIP d=400 pc; third body from light curva analysis (Equ_1); mass
S Equ    | transfer and third body from O-C analysis (Equ_7, Equ_8).
AS Eri   |HIP d=228 pc.
RW Gem   |HIP d=95 pc.
RX Gem   |Period change (Gem_14); third body (Gem_15); accretion disk (Gem_16,
RX Gem   | Gem_17).
RY Gem   |Accretion disk (Gem_18, Gem_17).
AF Gem   |Triple star (Gem_19).
AY Gem   |Period change (Gem_20).
BD Gem   |Accretion disk (Gem_17).
X Gru    |Period change  (Gru_1).
U Her    |HIP d=265(39) pc.
SZ Her   |HIP d=216(57) pc.
UX Her   |HIP d=209(50) pc.
V338 Her |HIP d=380(150) pc.
SX Hya   |HIP d= 245(71) pc.
TT Hya   |HIP d= 154(22) pc.
RT Lac   |RS CVn, third body, period change (Lac_12, Lac_13, Lac_14); the
RT Lac   | variation of orbital period shows a correlation with the activity
RT Lac   | level of the primary component (Lac_5).
UW Lac   |Apsidal motion (Lac_15).
AU Lac   |Eccentric orbit (Lac_16).
DG Lac   |Period change (Lac_3).
Y Leo    |HIP d=239(88) pc ; Orbital period is variable and O-C diagram shows
Y Leo    | sinusoidal variations (Leo_5,KKN).
UU Leo   |Orbital period variation (KKN).
VZ Leo   |Orbital period is variable and O-C shows parabolic variations
VZ Leo   | (KKN, Leo_6).
T LMi    |Orbital period variation (LMi_3, KKN).
RS Lep   |Orbital Period Variation (KKN).
Delta Lib|HIP d=93.3(7.9) pc, Apsidal Motion (Lib_3), Orbital period variation
Delta Lib| (KKN).
RV Lib   |HIP d=370(290) pc.
SS Lib   |HIP d=330(200) pc, Orbital period variation (KKN).
Beta Lyr |HIP d=270(38) pc; High rate mass transfer:2x10^-5^(M/year) (Lyr_1).
RV Lyr   |Orbital period variation (KKN).
TT Lyr   |Tycho d=91(66) pc.
EW Lyr   |Orbital period variation (KKN).
RW Mon   |HIP d=230(81), Orbital period variation (KKN).
TU Mon   |HIP d=370(170) pc.
AR Mon   |HIP d=276(93) pc.
AU Mon   |Circumstellar matter, presumably associated with the accretion disk
AU Mon   | (Mon_15).
BO Mon   |Orbital period variation (KKN).
V635 Mon |HIP d=330(110) pc.
V745 Mon |HIP d=249(66) pc, It was newly classified by Hipparcos.
UV Mus   |Tycho d=27(18) pc.
DZ Mus   |HIP d=321(97) pc.
RV Oph   |Magnetic activity (Oph_1).
RZ Oph   |HIP d= 430(380) pc : Accretion disk (Oph_6).
UU Oph   |HIP d= 139(37) pc .
DN Ori   |HIP d=390(180) pc, Accretion disk structure around the primary
DN Ori   | component (Ori_3).
EQ Ori   |Orbital period variation (KKN).
EY Ori   |HIP d=420(270) pc.
FH Ori   |Orbital period variation (KKN).
FK Ori   |Orbital period variation (KKN).
FL Ori   |Orbital period variation (KKN).
OS Ori   |Orbital period variation (KKN).
TY Peg   |HIP d= 230(88) pc.
AQ Peg   |HIP d= 490(420) pc.
AW Peg   |HIP d=160(24) pc.
DF Peg   |HIP d= 470(260) pc.
DI Peg   |HIP d=193(64) pc.
Beta Per |HIP d=28.46(0.73) pc ; Third body with mass 1.8 M and mass transfer
Beta Per | (Per_1) ; Asymetric transient accretion disk (Per_11).
Z Per    |Decreasing period and irregular period jumps (Per_17).
RT Per   |HIP d=180(70) pc; Period decrease and third body (Per_18).
RV Per   |Orbital period variation (KKN).
RW Per   |HIP d=290(120) pc; Disk structure (Per_8); Orbital period variation
RW Per   | (KKN).
RY Per   |HIP d=630(470) pc; The border between permanent and transient disk
RY Per   |(Per_3).
ST Per   |Orbital period variation (KKN), Third and forth body from orbital
ST Per   | period analysis (Per_19).
WY Per   |Orbital period variation (KKN).
XZ Per   |Orbital period variation (KKN).
DM Per   |HIP d=580(320) pc ; Triple system (Per_10).
V436 Per |HIP d=315 pc, Apsidal motion (Per_20).
Y Psc    |Orbital period is variable (Psc_4, KKN).
XZ Pup   |HIP d=253(66) pc; Orbital period variation (KKN).
V397 Pup |HIP d=147(11) pc, It was newly classified by HIPPARCOS.
U Sge    |HIP d=311(71) pc ; Orbital period variability due to apsidal
U Sge    | motion (Sge_3) ; It has a accretion disk around primary component
U Sge    | (Sge_4).
UZ Sge   |Orbital period variation (KKN).
RS Sgr   |HIP d=270(63)pc ; Increasing period due to the mass transfer (Sge_3),
RS Sgr   | Apsidal Motion (Sgr_8).
SX Sgr   |TYCHO d=40(32) pc .
WX Sgr   |Orbital period variation (KKN).
XY Sgr   |Orbital period variation (KKN).
XZ Sgr   |HIP d=234(78) pc; Orbital period variation (KKN).
EG Sgr   |Orbital period variation (KKN).
V356 Sgr |HIP d=600(360) pc.
V505 Sgr |HIP d=117(19) pc, Orbital period variation, third body (Sgr_10, KKN).
FV Sco   |HIP d=720(480) pc, new classified star, periodic variable; radio
FV Sco   | continuum emission (Sco_1); a microwave survey of southern active
FV Sco   | stars (Sco_2).
V393 Sco |HIP d=470(260) pc, new classified star, periodic variable; radio
V393 Sco | continuum emission (Sco_1); a microwave survey of southern active
V393 Sco | stars (Sco_2).
U Sct    |Orbital period variation (KKN).
RS Sct   |HIP d=260(110) pc, Orbital period variation (KKN).
RY Sct   |Disk structure (Sct_9), Orbital period variation (Sct_11, KKN).
RZ Sct   |HIP d=800(650) pc, Orbital period variation (KKN).
BS Sct   |Orbital period variation (KKN).
W Ser    |HIP d=370(180) pc, Orbital period variation (KKN).
AK Ser   |Orbital period variation (KKN).
AO Ser   |Orbital period variation (KKN).
Lamda Tau|HIP d=114 pc: Third body (Tau_9); apsidal motion (Tau_12).
RW Tau   |HIP d=300 pc; accertion disk (Tau_13).
AC Tau   |Period change, third body (Tau_12).
BN Tau   |Orbital period variation (KKN).
HU Tau   |HIP d=111(10) pc.
X Tri    |HIP d=166(35) pc .
TX UMa   |HIP d=211(48) pc ; Apsidal Motion (UMa_9); Accretion Disk Structure
TX UMa   |(UMa_10).
VV UMa   |O-C shows sinusoidal variation due to the third body (UMa_10).
XZ UMa   |Orbital period variation (KKN).
AC UMa   |Orbital period variation (KKN).
RW UMa   |HIP d=240(110) pc.
W UMi    |HIP d=450(150) pc ; Orbital period is variable (UMi_1; KKN).
RU UMi   |Large-scale spot activity on the secondary component(UMi_6), Orbital
RU UMi   | period variation (KKN).
TY UMi   |HIP d=109.9(7.1) pc, It was newly classified by Hipparcos.
S Vel    |HIP d=151(18) pc; Orbital period variation (KKN).
RX Vel   |TYCHO d=23.8(9.1) pc.
UW Vir   |HIP d=460(230) pc; Orbital period variation (KKN).
BD Vir   |HIP d=270(100) pc; Orbital period variation (KKN).
DL Vir   |HIP d=281(82) pc; Orbital period variation (KKN, Vir_1).
UY Vir   |HIP d=132(16) pc.
DM Vir   |HIP d=340(150) pc.
Z Vul    |HIP d=350(120) pc; Orbital period variation (KKN).
RS Vul   |HIP d=287(72) pc.
AX Vul   |Orbital period variation (KKN).
AY Vul   |Orbital period variation (KKN).
BO Vul   |Orbital period variation (KKN).
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