Elemental abundance analyses with DAO spectrograms: XXXI. The early F supergiants nu her (F2 II) and 41 cyg (F5 Ib-II)


Adelman S. J. , Cay I. H. , Tektunali H. G. , Gulliver A. F. , Teker A.

ASTRONOMISCHE NACHRICHTEN, cilt.329, ss.4-9, 2008 (SCI İndekslerine Giren Dergi) identifier identifier

  • Cilt numarası: 329 Konu: 1
  • Basım Tarihi: 2008
  • Doi Numarası: 10.1002/asna.200710863
  • Dergi Adı: ASTRONOMISCHE NACHRICHTEN
  • Sayfa Sayıları: ss.4-9

Özet

This series of high quality elemental abundance analyses of mostly Main Sequence normal and peculiar B, A, and F stars defines their properties and provides data for the comparison with analyses of somewhat similar stars and with theoretical predictions. Most use high dispersion and high S/N (>= 200) spectrograms obtained with CCD detectors at the long camera of the 1.22-m Dominion Astrophysical Observatory telescope's coude spectrograph. Here we expand the range of stars examined to include two relatively quiescent F supergiants. nu Her (F2 II) and 41 Cyg (F5 Ib-II) are analyzed as consistently as possible with previous studies. These LTE fine analyses use the ATLAS9 and the WIDTH9 programs of R. L. Kurucz. High signal-to-noise spectrograms and high quality atomic data were employed. The derived values of these photometrically constant stars are somewhat different with the abundances of v Her being somewhat metal-poor and those of 41 Cyg being crudely solar-like. Our analyses indicate that the basic results of Luck & Wepfer (1995) who also studied nu Her and 41 Cyg are not likely to be significantly changed by new studies of all their stars. (c) 2008 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.