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II/180          uvby-beta photometry of metal-poor stars (Schuster+ 1989)

uvby-beta photometry of high-Velocity and metal-poor stars Schuster W.J., Nissen P.E. <Astron. Astrophys. 222, 69 (1989)> =1989A&A...222...69S
ADC_Keywords: Stars, high-velocity ; Stars, metal-deficient Keywords: evolution of the Galaxy - halo stars - metallicity - ages Description: Using the calibrations derived by Schuster and Nissen (=1989A&A...221...65S), the interstellar color excesses, E(b-y), and the metallicities, [Fe/H], have been determined for the 711 high velocity and metal-poor stars in the catalogue of uvby-beta photometry (=1988A&AS...73..225S). 220 of these listed in table1 turn out to be halo stars according to the criterion [Fe/H] ≤ -1.0. About 15% of the halo stars have colors that are significantly affected by interstellar reddening, i.e. E(b-y) > 0.025. The distributions in the c0-(b-y)0 diagram of the halo stars grouped according to [Fe/H], have well defined turn-off points. From the Teff values of these points a minimum age of 18-20 Gyr for the halo stars is determined. However, this age may be 2-3 Gyr too high due to a possible systematic error in Teff for the stellar models used. Relative ages of 77 halo stars in the turn-off region of the c0-(b-y)0 diagram are derived using the isochrones VandenBerg and Bell (=1985ApJS...58..561V). Assuming that the O/Fe abundance ratio is constant in halo stars, evidence of a cosmic age scatter of ±2.5Gyr at a given metallicity is found. Furthermore, the mean age of the halo stars is found to decrease smoothly by about 3 Gyr from [Fe/H]= -2.0 to -1.0. These results suggest that a pressure-supported slow uniform collapse controlled the formation and early evolution of the Galaxy. However, the scenario of Searle and Zinn (=1978ApJ...225..357S) is also compatible with the results. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table1 73 220 The Catalogue
See also: J/A+AS/97/951 : Metal-poor stars uvby-beta photometry. VI. (Schuster+, 1993) J/A+AS/117/317 : Metal-poor stars uvby-beta photometry. VIII. (Schuster+, 1996) 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
3- 12 A10 --- Name Star designation (HD/DM/Giclas) 15- 16 I2 h RAh Right Ascension 1950 18- 19 I2 min RAm Right Ascension 1950 21- 24 F4.1 s RAs Right Ascension 1950 27 A1 --- DE- Declination 1950 Sign 28- 29 I2 deg DEd Declination 1950 31- 32 I2 arcmin DEm Declination 1950 34- 35 I2 arcsec DEs Declination 1950 38- 43 F6.3 mag E(b-y) ? Interstellar reddening 45 A1 --- l_[Fe/H] '<' if [Fe/H] metallicity is an upper limit 46- 50 F5.2 Sun [Fe/H] [-3.5/-1[ Metallicity (relative to Sun) 53- 56 F4.1 Ga Age ? Age in Giga-years 59- 61 F3.1 Ga e_Age ? rms error on Age 64- 73 A10 --- Notes Remarks (1)
Note (1): the following symbols are used in the remarks: AGB = asymptotic giant branch D = two stars in the diaphragm PHV = photometrically variable RHB = red horizontal branch RV-var = radial velocity variable SB-CL = spectroscopic binary (Carney + Latham, 1987, AJ 93, 116) SG = subgiant BS? = possible blue straggler * See Individual Notes
Individual Notes: G 266-060: common proper motion with G 226-061. HD 23439: double, component B is SB-CL, orbital elements by Latham et al. (=1988AJ.....96..567L). G 088-010: orbital elements by Latham et al. (=1988AJ.....96..567L). G 089-014: orbital elements by Latham et al. (=1988AJ.....96..567L). G 114-026: orbital elements by Latham et al. (=1988AJ.....96..567L). HD 103095: double, orbital elements by Beardsley et al. (=1974ApJ...194..637B). G 065-022: orbital elements by Latham et al. (=1988AJ.....96..567L). HD 134439: common proper motion with HD 134440. G 141-019: orbital elements by Latham et al. (=1988AJ.....96..567L). G 206-034: orbital elements by Latham et al. (=1988AJ.....96..567L). G 026-009: double lined SB, orbital elements by Peterson et al. (=1980ApJ...239...50R). G 126-062: orbital elements by Latham et al. (=1988AJ.....96..567L). Acknowledgements: We thank Dr Poul E. Nissen for having supplied a copy of Table1. Historical Notes: * 09-Sep-1992: table supplied by Poul E. Nissen * 04-Jan-1993: First documentation at CDS (Francois Ochsenbein) * 03-Nov-1995: Documentation standardized at CDS, and notes added (Francois Ochsenbein) References: Schuster et al., Paper I 1988A&AS...73..225S Schuster et al., Paper II 1989A&A...221...65S 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 et al., Paper VIII 1996A&AS..117..317S, Cat. J/A+AS/117/317 Schuster et al., Paper IX 1997A&A...319..796S Schuster et al., Paper X 2004A&A...422..527S, Cat. J/A+A/422/527 Schuster et al., Paper XI 2006A&A...445..939S, Cat. J/A+A/445/939
(End) Francois Ochsenbein [CDS] 03-Nov-1995
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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