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, vol.16, no.3, pp.191-193, 2011 (SCI-Expanded) identifier identifier

  • Publication Type: Article / Article
  • Volume: 16 Issue: 3
  • Publication Date: 2011
  • Doi Number: 10.1016/j.newast.2010.09.009
  • Journal Name: NEW ASTRONOMY
  • Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Page Numbers: pp.191-193
  • Keywords: 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 University Affiliated: Yes

Abstract

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.