Elemental abundance analyses with DAO spectrograms. XXVIII. Comparisons with two series of automated elemental abundance analyses

YÜCE K., Adelman S. J., Gulliver A. F.

NEW ASTRONOMY, cilt.16, sa.3, ss.191-193, 2011 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 16 Sayı: 3
  • Basım Tarihi: 2011
  • Doi Numarası: 10.1016/j.newast.2010.09.009
  • Dergi Adı: NEW ASTRONOMY
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.191-193
  • Anahtar Kelimeler: Stars: abundances, Stars: atmosphere parameters, Stars: individual (Vega, is an element of Aqr, theta And, 2 Lyn, gamma Gem, lambda UMa, beta UMa, theta Leo, 29 Vul, o Peg, delta Aqr, xi(2) Cet, sigma Boo, is an element of Ser, 101 Her, pi Dra, 29 Cyg, sigma Aqr), A-TYPE STARS, COMPOSITIONAL DIFFERENCES, ASTRA SPECTROPHOTORNETER, DISTRIBUTION GEOMETRY, MAGNETIC-FIELD, IOTA, VULPECULAE, SERPENTIS, HERCULIS, PECULIAR
  • Ankara Üniversitesi Adresli: Evet

Özet

We compare the results of our series of fine analyses based on Dominion Astrophysical Observatory long camera coude spectra with those of the same stars from the series of automated elemental abundance analyses by Hill (1995) and by Erspamer and North (2003). We usually find good agreement with the results of the first paper for those elements with well-determined abundances and somewhat poorer agreement with results of the second paper. (C) Elsevier B.V. All rights reserved.