J/AJ/117/2329  Spectroscopy of hot stars in the halo. III   (Wilhelm+, 1999)

Spectroscopy of hot stars in the galactic halo. III. Analysis of a large sample of field horizontal-branch and other A-type stars Wilhelm R., Beers T.C., Sommer-Larsen J., Pier J.R., Layden A.C., Flynn C., Rossi S., Christensen P.R. <Astron. J. 117, 2329 (1999)> =1999AJ....117.2329W 1999AJ....117.2329W
ADC_Keywords: Abundances, [Fe/H] ; Photometry, UBV ; Stars, horizontal branch Keywords: Galaxy: halo - stars: horizontal-branch - stars: Population II Abstract: We present results from an analysis of medium-resolution spectroscopy and UBV photometry for a sample of 1121 A-type stars in the halo (and disk) of the Galaxy. A previously developed calibration technique is used to assign estimates of effective temperature, surface gravity, and stellar metal abundance, as parametrized by [Fe/H]. Radial velocities are reported with an accuracy of ∼10 km.s-1. Distance estimates are obtained for the stars with well-determined luminosity classes. Note that although we refer to "A-type" stars, which dominate the present sample, the present data set includes roughly 100 stars of later spectral types, as a result of the temperature range we have chosen to explore in this paper (6000 K ≤ Teff ≤ 10,000 K). File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 106 1121 Observed properties of the program sample table2a.dat 80 140 Physical parameters for the Am/Ap subsample table2b.dat 83 444 Physical parameters for the FHB subsample table2c.dat 82 416 Physical parameters for the A V subsample table2d.dat 83 121 Physical parameters for the FHB/A subsample table3.dat 30 19 Known variable stars tablea1.dat 52 58 Additional photometry for hot star candidates tableb1.dat 45 81 Program stars with duplicate HK survey identifications -------------------------------------------------------------------------------- See also: J/AJ/87/1515 : UBV photometry of AB stars in halo (Pier, 1982) J/ApJS/53/791 : Spectroscopy of AB stars in halo (Pier, 1983) J/AJ/90/2089 : Stars of very low metal abundance. (Beers+, 1985) J/PASP/102/1392 : UBV photometry from HK survey. (Doinidis+ 1990) J/PASP/103/973 : Photoelectric UBV from HK survey. (Doidinis+ 1991) J/ApJS/76/1001 : UBV photometry of HK survey stars (Preston+, 1991) J/AJ/103/267 : Spectrocopy of hot stars in galactic halo (Beers+ 1992) J/AJ/103/1987 : Stars of very low metal abundance (Beers+ 1992) J/AJ/108/268 : HK survey emission-line candidates positions (Beers+ 1994) J/AJ/108/538 : Metal-poor MS stars UBV photometry (Preston+ 1994) J/AJ/112/1188 : HK survey emission-line candidates (Beers+ 1996) J/ApJS/123/639 : UBV photometry of metal-weak candidates (Norris+, 1999) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- BPS Star Name (field-number) 15 A1 --- f_BPS [ab] Flag indicating new photometry (1) 19- 20 I2 h RAh Right Ascension (B1950) 22- 23 I2 min RAm Right Ascension (B1950) 25- 28 F4.1 s RAs Right Ascension (B1950) 30 A1 --- DE- Sign of the Declination (B1950) 31- 32 I2 deg DEd Declination (B1950) 34- 35 I2 arcmin DEm Declination (B1950) 37- 38 I2 arcsec DEs Declination (B1950) 40- 44 F5.2 mag Vmag V band magnitude 46- 50 F5.2 mag B-V The B-V color 55- 59 F5.2 mag U-B ? The U-B color 61- 65 F5.2 mag E(B-V) The B-V reddening 71- 74 F4.1 0.1nm EqWK ? Equivalent width of the CaII K line 76- 79 F4.1 0.1nm Ddelta Line width of Hδ at 20% below the local continuum level 81- 84 F4.1 0.1nm Dgamma Line width of Hγ at 20% below the local continuum level 87- 90 I4 km/s Vhelio Heliocentric radial velocity 92 A1 --- u_Vhelio Indicates an uncertain radial velocity 95 A1 --- Obs1 Observatory's code where data was obtained (2) 97 A1 --- Obs2 Second observatory's code where data was obtained (2) 99 A1 --- Obs3 Third observatory's code where data was obtained (2) 101-108 A8 --- Class MK Stellar classification -------------------------------------------------------------------------------- Note (1): a = New CTIO photometry b = New Siding Spring Observatory photometry by Norris, Ryan, & Beers (1999ApJS..123..639N 1999ApJS..123..639N) Note (2): E = European Southern Observatory H = Beers et al. (1992AJ....103..267B 1992AJ....103..267B) K = Kitt Peak National Observatory L = Lowell observatory -------------------------------------------------------------------------------- Byte-by-byte Description of file: table2?.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- BPS Star name 16- 20 I5 K Teff Effective temperature 22 A1 --- u_Teff Uncertain Teff flag 26- 28 F3.1 [cm/s2] log(g) The log of the surface gravity 30 A1 --- u_log(g) Uncertain log(g) flag 36- 39 F4.1 [Sun] Wk ? The [Fe/H] abundance from the CaII K-line equivalent width technique 43- 46 F4.1 [Sun] CTA ? The [Fe/H] abundance from the CaII K template matching technique 50- 53 F4.1 [Sun] MTA ? The [Fe/H] abundance from the metallic- line region template matching procedure 55 A1 --- u_MTA Uncertain MTA flag 57- 60 F4.1 [Sun] AVG ? Average [Fe/H] abundance from best estimate 62 A1 --- u_AVG Abundance obtained from Lowell data 65- 67 F3.1 [Sun] Diff ? Absolute difference between the two most consistent metallicity indicators 71- 74 F4.1 kpc Dist ? Distance estimate 79- 83 A5 --- Text Comment on star (1) -------------------------------------------------------------------------------- Note (1): abbreviations are: r = Noted in present analysis as a candidate variable star rr = noted by Preston et al. (1991ApJS...76.1001P 1991ApJS...76.1001P) as a candidate variable star RR = noted in Table 3 as an RR Lyrae variable B = classified by Preston et al. (J/AJ/108/538) as a BMP star -------------------------------------------------------------------------------- Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- BPS CS designation 15- 23 A9 --- OtherName Other Name 26- 30 A5 --- Class Class -------------------------------------------------------------------------------- Byte-by-byte Description of file: tablea1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- BPS CS designation 15- 16 I2 h RAh Right ascension (1950.0) 18- 19 I2 min RAm Right ascension (1950.0) 21- 24 F4.1 s RAs Right ascension (1950.0) 26 A1 --- DE- Declination sign (1950.0) 27- 28 I2 deg DEd Declination (1950.0) 30- 31 I2 arcmin DEm Declination (1950.0) 33- 34 I2 arcsec DEs Declination (1950.0) 36- 40 F5.2 mag Vmag V magnitude 42- 46 F5.2 mag B-V B-V colour index 48- 52 F5.2 mag U-B U-B colour index -------------------------------------------------------------------------------- Byte-by-byte Description of file: tableb1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 13 A13 --- BPS Catalogued star name 17- 29 A13 --- BPS1 Alternate name 1 33- 45 A13 --- BPS2 Alternate name 2 -------------------------------------------------------------------------------- History: From AJ electronic edition. References: (Paper II) Wilhelm+ 1999AJ....117.2308W 1999AJ....117.2308W (Paper I) Beers+ 1992AJ....103..267B 1992AJ....103..267B
(End) Greg Schwarz [AAS] 25-Apr-2000
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