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J/A+AS/127/277 Rotation and binary rate among giant F stars (Kunzli+ 1998)
Are metallic A-F giants evolved Am stars? Rotation and rate of binaries among giant F stars Kuenzli M., North P. <Astron. Astrophys. Suppl. Ser. 127, 277 (1998)> =1998A&AS..127..277K (SIMBAD/NED BibCode)
ADC_Keywords: Binaries, spectroscopic ; Stars, F-type ; Stars, giant ; Radial velocities Keywords: stars: binaries: spectroscopic - stars: chemically peculiar - stars: evolution - stars: rotation - stars: Delta Scuti Description: We have tested the hypothesis of Berthet (1991A&A...251..171B) which foresees that Am stars become giant metallic A and F stars (defined by an enhanced value of the blanketing parameter δm2 of the Geneva photometry) when they evolved. If this hypothesis is right, Am and metallic A-FIII stars need to have the same rate of binaries and a similar distribution of vsini. From our new spectroscopic data and from vsini and radial velocities in the literature, we show that it is not the case. The metallic giant stars are often fast rotators with vsini larger than 100 km/s, while the maximum rotational velocity for Am stars is about 100 km/s. The rate of tight binaries with periods less than 1000 days is less than 30 % among metallic giants, which is incompatible with the value of 75 % for Am stars (Abt & Levy, 1985ApJS...59..229A). Therefore, the simplest way to explain the existence of giant metallic F stars is to suggest that all normal A and early F stars might go through a short "metallic" phase when they are finishing their life on the main sequence. Besides, it is shown that only giant stars with spectral type comprised between F0 and F6 may have a really enhanced δm2 value, while all A-type giants seem to be normal. File Summary:
FileName Lrecl Records Explanations
ReadMe 80 . This file table2 30 54 Radial velocities of standard stars table3 30 236 Radial velocities of A and F giants table6 80 148 Discussion about the duplicity of all photometric metallic F giant stars of Hauck (1986A&A...155..371H) tables.tex 147 901 LaTeX version of the tables
Byte-by-byte Description of file: table2 table3
Bytes Format Units Label Explanations
1- 6 I6 --- HD HD number (1) 8- 18 F11.3 d HJD Heliocentric Julian day 20- 25 F6.2 km/s RV Radial velocity 27- 30 F4.2 km/s e_RV rms uncertainty on RV
Note (1): Average values of radial velocity for table2 stars: ------------------------ Star <Vr> ------------------------ HD 693 15.44±0.36 HD 22484 27.86±0.44 HD 89449 5.84±0.52 HD 114762 47.77±0.26 HD 136202 54.39±0.27 HD 187691 -0.27±0.49 HD 222368 5.12±0.45 ------------------------
Byte-by-byte Description of file: table6
Bytes Format Units Label Explanations
1- 6 I6 --- Name ? HD number 8- 9 I2 --- NTot Total number of lines for the reference 11- 12 I2 --- Nline Running line number in range [1,Ntot] 14- 80 A67 --- Com Comments (1)
Note (1): References: Abt (1965ApJS...11..429A) Abt (1969ApJS...19..387A) Abt & Biggs, 1972, Bibliography of Stellar Radial Velocities, Latham Process Corp., New York Abt & Levy (1976ApJS...30..273A) Adams et al. (1929ApJ....70..207A) Breger (1979PASP...91....5B) Buscombe & Morris (1958MNRAS.118..609B) Campbell (1913LicOB...7..113C) Campbell (1928PLicO..16.....C) Cannon (1920PDO.....4..253C) Catchpole et al. (1982RGOB..188....5C) Evans (1961RGOB...44..351E) Evans (1966RGOB..110..185E) Evans et al. (1961RGOB...48..389E) Evans et al. (1964RGOB...85..207E) Evans et al. (1957MNRAS.117..534E) Frost et al. (1929PYerO...7....1F) Harper (1937PDAO....7....1H) Henroteau (1923PDO.....8...59H) Jones & Haslam (1969RGOB..155...19J) Mayor & Mazeh (1987A&A...171..157M) Nelson & Kreidl (1993AJ....105.1903N) Neubauer (1930LicOB..15...47N) Nordstroem & Andersen (1985A&AS...61...53N, Cat. III/127) Penfold (1971PASP...83..497P) Rodriguez et al. (1994A&AS..106...21R) Rosvick & Scarfe (1991PASP..103..628R) Sanford & Karr (1942ApJ....96..214S) Shajn & Albitzky (1932MNRAS..92..771S) Smith (1982ApJ...254..242S) Wilson & Joy (1950ApJ...111..221W) Wooley et al. (1971ROAn...14....1W)
Acknowledgements: Marc Kunzli
(End) Francois Ochsenbein [CDS] 15-Jul-1997
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