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Elemental abundance analyses with DAO spectrograms. XXVIII. Comparisons with two series of automated elemental abundance analyses |
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| Authors: | K. Yüce S.J. Adelman A.F. Gulliver |
| Affiliation: | 1. Ankara University, Faculty of Science, Department of Astronomy and Space Sciences, TR-06100, Tando?an, Ankara, Turkey;2. Istituto Nazionale di Astrofisica-Osservatorio Astronomico di Trieste, via G.B. Tiepolo, 11, I-34143 Trieste, Italy;3. Department of Physics, The Citadel, 171 Moultrie Street, Charleston, SC 29409, United States;4. Visiting Astronomer, Dominion Astrophysical Observatory, Herzberg Institute of Astrophysics, National Research Council of Canada, 5071 W. Saanich Road, Victoria, Canada V8X 4M6;5. Department of Physics and Astronomy, Brandon University, Brandon, Canada MB R7A 6A9 |
| Abstract: | 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. |
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