Elemental abundance analyses with DAO spectrograms .16. The normal F main-sequence stars sigma Bootis, theta Cygni and iota Piscum, and the Am stars 15 Vulpeculae and 32 Aquarii


Creative Commons License

ADELMAN S., Caliskan H. , KOÇER D., BOLCAL Ç.

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.288, ss.470-500, 1997 (SCI İndekslerine Giren Dergi)

  • Cilt numarası: 288 Konu: 2
  • Basım Tarihi: 1997
  • Doi Numarası: 10.1093/mnras/288.2.470
  • Dergi Adı: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
  • Sayfa Sayısı: ss.470-500

Özet

Elemental abundances of the sharp-lined F2 V star sigma Boo are derived consistent with other studies of this series of papers. Previous studies of the F4 V star theta Cyg and the F7 V star iota Psc and of the Am stars 15 Vul and 32 Aqr are revised and extended. The normal stars have microturbulences between 1.2 and 1.6 km s(-1), while the Am stars have values between 4.0 and 4.5 km s(-1). Most derived abundances for a Cyg are close to solar as are those for iota Psc, except for the rare earth elements which are enhanced. sigma Boo, however, is a marginally metal-poor star. The abundances of 15 Vul indicate it is a marginal Am star while those of 32 Aqr exhibit the Am phenomenon to a greater extent.