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J/A+AS/125/313 RR Lyrae radial velocities and [Fe/H] I. (Fernley+ 1997)
Radial velocities and iron abundances of field RR Lyraes. I. Fernley J., Barnes T.G. <Astron. Astrophys. Suppl. Ser. 125, 313 (1997)> =1997A&AS..125..313F (SIMBAD/NED BibCode)
ADC_Keywords: Stars, variable ; Abundances, [Fe/H] ; Radial velocities Keywords: stars: abundances ; V363 Cas ; AT And - stars: binaries: spectroscopic - stars: variables - stars: kinematics Abstract: We present systemic velocities and iron abundances for 56 RR Lyraes, the majority of which have been observed by the HIPPARCOS satellite. Comparison between our systemic velocities and previous values identifies several binary candidates only one of which, TU UMa, was previously suspected of being a binary. However, spectra of the unusual RR Lyrae BB Vir show no evidence of line doubling and hence do not support the recent claims that this star may have a Blue Horizontal Branch companion. Comparison between our abundances and previous determinations shows reasonable agreement except with the recent work of Layden (1994, Cat. J/AJ/108/1016) where we find systematic differences. Several of the stars included on the HIPPARCOS observing list as RR Lyraes are shown to be mis-classified. Of particular interest are the stars V363 Cas and AT And which, by analogy with XZ Cet, may be anomalous Cepheids. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file appen.dat 142 56 Radial velocities and metal abundances of RR Lyr appen.tex 118 188 LaTeX version of appen
See also: J/A+AS/125/321 : RR Lyrae radial velocities and [Fe/H] II. (Solano+ 1997) Byte-by-byte Description of file: appen.dat
Bytes Format Units Label Explanations
1- 8 A8 --- Name Star name 10- 11 I2 h RAh Right Ascension J2000 (hours) (5) 13- 14 I2 min RAm Right Ascension J2000 (minutes) (5) 16- 17 I2 s RAs Right Ascension J2000 (seconds) (5) 19 A1 --- DE- Declination J2000 (sign) (5) 20- 21 I2 deg DEd Declination J2000 (degrees) (5) 23- 26 F4.1 arcmin DEm Declination J2000 (minutes) (5) 28- 35 F8.6 d Per ? Pulsation period 36 A1 --- Note [c*&] Note on star (1) 38- 42 F5.2 Sun [Fe/H] ? Abundance calculated in this work 44- 48 F5.2 Sun [Fe/H]1 ? Abundance taken from the literature (2) 50 I1 --- r_[Fe/H]1 ? [1/9] Reference for [Fe/H]1 (3) 52- 56 F5.2 Sun [Fe/H]2 ? Abundance taken from the literature (2) 58 I1 --- r_[Fe/H]2 ? [1/9] Reference for [Fe/H]2 (3) 60- 64 F5.2 Sun [Fe/H]3 ? Abundance taken from the literature (2) 66 I1 --- r_[Fe/H]3 ? [1/9] Reference for [Fe/H]3 (3) 68- 72 F5.2 Sun [Fe/H]4 ? Abundance taken from the literature (2) 74- 75 I2 --- r_[Fe/H]4 ? [1/10] Reference for [Fe/H]4 (3) 77- 81 F5.2 Sun [Fe/H]5 ? Abundance taken from the literature (2) 83- 84 I2 --- r_[Fe/H]5 ? [1/10] Reference for [Fe/H]5 (3) 86- 90 F5.2 Sun [Fe/H]6 ? Abundance taken from the literature (2) 92 I1 --- r_[Fe/H]6 ? [1/9] Reference for [Fe/H]6 (3) 94- 97 I4 km/s Vsys Systemic velocity calculated in this work 99-100 I2 km/s e_Vsys rms uncertainty on Vsys 102-105 I4 km/s Vsys1 ? Systemic velocity taken from the literature 107-108 I2 km/s e_Vsys1 ? rms uncertainty on Vsys1 110-111 I2 --- r_Vsys1 ? [1/21] Reference for Vsys1 (4) 113-116 I4 km/s Vsys2 ? Systemic velocity taken from the literature 118-119 I2 km/s e_Vsys2 ? rms uncertainty on Vsys2 121-122 I2 --- r_Vsys2 ? [1/21] Reference for Vsys2 (4) 124-127 I4 km/s Vsys3 ? Systemic velocity taken from the literature 129-130 I2 km/s e_Vsys3 ? rms uncertainty on Vsys3 132-133 I2 --- r_Vsys3 ? [1/21] Reference for Vsys3 (4) 135-136 I2 km/s Vsys4 ? Systemic velocity taken from the literature 138 I1 km/s e_Vsys4 ? rms uncertainty on Vsys4 140-141 I2 --- r_Vsys4 ? [1/21] Reference for Vsys1 (4)
Note (1): *: See Section 5 for a discussion of this star for which the classification as an RR Lyrae is uncertain &: only one observation of this star was made; hence the larger errors. Based on the large amplitude shown in the GCVS it is assumed to be an 'ab' type c: c-type, blank indicates ab-type Note (2): {DELTA}S values from previous work have been transformed to [Fe/H] using [Fe/H] = -0.13-0.195{DELTA}S (Fernley & Barnes 1996). As discussed in the text, the uncertainty in the [Fe/H] values, both from previous work and this work, is typically ±0.13 dex. Note (3): Sources of abundances: 1: Butler (1975ApJ...200...68B) 2: Kemper (1982AJ.....87.1395K) 3: Preston (1959ApJ...130..507P) 4: Clementini et al. (1991AJ....101.2168C) 5: Kinman & Caretta (1992PASP..104..111K) 6: Smith (1990PASP..102..124S) 7: Suntzeff et al. (1991ApJ...367..528S) 8: Layden (1994AJ....108.1016L), Cat. J/AJ/108/1016 9: Lambert et al. (1996ApJS..103..183L) 10: Clementini et al. (1995AJ....110.2319C), Cat. J/AJ/110/2319 Note (4): Sources of mean radial velocities: 1: Liu & Janes (1990ApJ...354..273L) 2: Jones et al. (1988ApJ...332..206J) 3: Hawley & Barnes (1985PASP...97..551H) 4: Woolley & Ali (1966RGOB..114....1W) 5: Farquhar (1948ApJ...107..276F) 6: Rogers (1960Obs....80..220R) 7: Varsavsky (1960ApJ...131..623V) 8: Cacciari et al. (1987A&AS...69..135C) 9: Burki & Meylan (1986A&A...156..131B) 10: Barnes et al. (1988ApJS...67..403B) 11: Layden (1994AJ....108.1016L), Cat J/AJ/108/1016 12: Imbert (1980A&A....86..259I) 13: Preston et al. (1961ApJ...133..484P) 14: Saha & White (1990PASP..102..148S) 15: Payne-Gaposhkin (1954AnHar.113....3P) 16: Woolley and Savage (1971RGOB..170....1W) 17: Joy (1938PASP...50..302J) 18: Joy (1950PASP...62...60J) 19: Joy (1955PASP...67..420J) 20: Preston (1959ApJ...130..507P) 21: Notni 1956, mitt. Jena No. 26 Note (5): Position added to the original table (taken from SIMBAD)
Acknowledgements: Enrique Solano
(End) Patricia Bauer [CDS] 18-Feb-1997
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