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J/A+AS/117/317 uvby-beta photometry of metal-poor stars. VIII. (Schuster+ 1996)

uvby-β photometry of high-velocity and metal-poor stars. VIII. Stars of very low metal abundance. Schuster W.J., Nissen P.E., Parrao L., Beers T.C., Overgaard L.P. <Astron. Astrophys. Suppl. Ser. 117, 317 (1996)> =1996A&AS..117..317S (SIMBAD/NED BibCode)
ADC_Keywords: Stars, high-velocity ; Stars, metal-deficient ; Photometry, uvby, beta ; Abundances, [Fe/H] Keywords: stars: abundances - stars: distances - stars: fundamental parameters - dust, extinction - Galaxy: evolution - Galaxy: halo Abstract: A catalogue of uvby-β photometry for 87 of the turn-off and subgiant stars from the HK survey of Beers et al. (1992AJ....103.1987B, BPSII) is given. Most of these stars have [Fe/H]≤2.5. These photometric data have been taken and reduced using the same techniques as in our previous two uvby-β catalogues (Schuster et al., 1989, Cat. II/180 and Schuster et al., 1993, Cat. J/A+AS/97/951). An error analysis has been made; typical mean observational errors for a star with V=14.2m are 0.008, 0.007, 0.011, 0.010 and 0.012 in V, (b-y), m1, c1 and β, respectively. Our photometric data are also compared to the UBV photometry and spectral indices from the HK survey; satisfactory agreement is found indicating good quality for the two data sets. The stars are classified in reddening-free diagrams of the uvby-β system; several of the stars are found to have been mis-classified in the HK survey. Two metal-poor supergiants, three (possibly four) horizontal branch stars, one blue subluminous star and two stars with ambiguous photometry have been identified. Stellar parameters, such as E(b-y), MV, δMV, and Teff, plus error estimates for these parameters, are provided using our photometric calibrations. Although all stars have galactic latitudes |b|≥30° many of them are significantly reddened with E(b-y) ranging from 0.02 to 0.15. The average reddening towards the South Galactic Pole region, b←60°, is E(b-y)=0.027±0.004 corresponding to E(B-V)=0.036±0.005 in contrast to the low value of E(B-V)∼0.01 derived from the Burstein & Heiles (1982AJ.....87.1165B) maps. The stars are analyzed in the (b-y)0, [Fe/H] diagram, and individual ages estimated using the isochrones of VandenBerg & Bell (1985ApJS...58..561V) and of Bergbusch & VandenBerg (1992ApJS...81..163B). These very metal-poor stars are found to be coeval, within 1-2Gyr, with the halo and thick-disk stars studied previously, with a mean age in excess of 18Gyr. Several blue "thick-disk" stars, which are perhaps analogous to the "blue metal-poor" stars of Preston et al. (1994, Cat. J/AJ/108/538), have been identified. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 80 87 The standard uvby-β catalogue for the 87 BPSII (Beers et al., 1992AJ....103.1987B) stars table2 70 86 Stellar parameters for the 86 VMP stars.
See also: II/180 : uvby-beta photometry of metal-poor stars. III. (Schuster+ 1989) J/A+AS/97/951 : uvby-beta photometry of metal-poor stars. VI. (Schuster+ 1993) J/AJ/103/1987 : Stars of very low metal abundance (Beers+ 1992) J/A+A/422/527 : Metal-poor stars uvby-beta photometry. X. (Schuster+, 2004) J/A+A/445/939 : Metal-poor stars uvby-beta photometry. XI. (Schuster+, 2006) Byte-by-byte Description of file: table1
Bytes Format Units Label Explanations
1- 9 A9 --- Star Star designation according to BPSII (Beers et al., 1992AJ....103.1987B) 11- 16 F6.3 mag Vmag V magnitude 18- 22 F5.3 mag b-y b-y colour index 24- 29 F6.3 mag m1 m1 colour index 31- 35 F5.3 mag c1 c1 colour index 37 I1 --- o_b-y Number of independent uvby observations 39- 43 F5.3 mag beta beta colour index 45 I1 --- o_beta Number of independent beta observations 47- 80 A34 --- Note Note
Byte-by-byte Description of file: table2
Bytes Format Units Label Explanations
1- 9 A9 --- Star Star designation according to BPSII (Beers et al., 1992AJ....103.1987B) 11- 16 F6.3 mag E(b-y) ? Reddening 18- 22 F5.3 mag e_E(b-y) ? rms uncertainty on E(b-y) 24- 28 F5.2 [Sun] [Fe/H]c ? Spectroscopic metallicity 30- 34 F5.2 [Sun] [Fe/H]p ? Photometric metallicity 35 A1 --- u_[Fe/H]p Uncertainty flag on [Fe/H]p 37- 40 F4.2 [Sun] e_[Fe/H]p ? rms uncertainty on [Fe/H]p 42- 45 F4.2 mag MV ? Absolute V magnitude 47- 50 F4.2 mag e_MV ? rms uncertainty on MV 52- 56 F5.2 mag dMV ? Evolutionnary correction δMV (See Nissen et al., 1991A&A...251..457N) 58- 61 F4.2 mag e_dMV ? rms uncertainty on dMV 63- 66 I4 K Teff ? Effective temperature 68- 70 I3 K e_Teff ? rms uncertainty on Teff
History: Prepared via OCR at CDS. References: Schuster at al., Paper I. 1988A&AS...73..225S Schuster at al., Paper II. 1989A&A...221...65S Schuster at al., Paper III. 1989A&A...222...69S, Cat. II/180 Allen et al., Paper IV. 1991A&A...244..280A Nissen et al., Paper V. 1991A&A...251..457N Schuster et al. Paper VI. 1993A&AS...97..951S, Cat. J/A+AS/97/951 Marquez et al., Paper VII. 1994A&AS..108..341M Schuster at al., Paper IX. 1997A&A...319..796S Schuster at al., Paper X. 2004A&A...422..527S, Cat. J/A+A/422/527 Schuster at al., Paper XI. 2006A&A...445..939S, Cat. J/A+A/445/939
(End) James Marcout, Patricia Bauer [CDS] 12-Sep-1997
The document above follows the rules of the Standard Description for Astronomical Catalogues.From this documentation it is possible to generate f77 program to load files into arrays or line by line

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