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

We compare the results of our series of fine analyses based on Dominion Astrophysical Observatory long camera coudé 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...

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Bibliographic Details
Published in:New astronomy 2011-04, Vol.16 (3), p.191-193
Main Authors: Yüce, K., Adelman, S.J., Gulliver, A.F.
Format: Article
Language:English
Subjects:
Stars: abundances
Stars: atmosphere parameters
Stars: individual (Vega, ϵ Aqr, θ And, 2 Lyn, γ Gem, λ UMa, β UMa, θ Leo, 29 Vul, o Peg, δ Aqr, ξ2 Cet, σ Boo, ϵ Ser, 101 Her, π Dra, 29 Cyg, σ Aqr)
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Summary:We compare the results of our series of fine analyses based on Dominion Astrophysical Observatory long camera coudé 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.
ISSN:1384-1076
1384-1092
DOI:10.1016/j.newast.2010.09.009