Astron. Astrophys. Suppl. Ser.
Volume 136, Number 3, May I 1999
|Page(s)||453 - 454|
|Published online||15 May 1999|
An abundance analysis of the single-lined spectroscopic binaries with barium stars-like orbital elements*
II. The spectroscopic data
Ventspils International Radio Astronomy Center, Akadēmijas laukums 1, LV-1050 Rīga, Latvia
2 Special Astrophysical Observatory, 357147 Nizhny Arkhyz, Russia
3 Department of Astronomy, Kazan State University, 420008 Kazan, Russia
Send offprint request to: L. Začs
Accepted: 21 January 1999
High–resolution spectroscopic observations are presented for 19 single–lined binaries (giants and dwarfs) with orbital elements and mass functions similar to those of barium stars, two radial velocity non–variable barium stars, and two standards. All binary systems contain an unseen low–mass component, presumably, a white dwarf. The equivalent widths and oscillator strengths are given for all measured spectral lines.
Key words: binaries: spectroscopic / stars: chemically peculiar / stars: abundances
Tables 2 and 3 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (22.214.171.124) or via http://cdsweb.u-strasbg.fr/Abstract.html
© European Southern Observatory (ESO), 1999