Astronomy and Astrophysics – Astrophysics
Scientific paper
Jul 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26as...70...49k&link_type=abstract
Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 70, no. 1, July 1987, p. 49-56. Research supported by the Ci
Astronomy and Astrophysics
Astrophysics
8
A Stars, B Stars, Metallic Stars, Stellar Composition, Stellar Spectra, Abundance, Astronomical Photography, Atmospheric Models, Spectrograms, Tables (Data)
Scientific paper
An abundance analysis using photographic region spectrograms and fully line-blanketed model atmospheres has been performed for the metallic-lined (Am) star 32 Aquarii consistent with previous papers of this series. Its pattern of abundance anomalies is not identical with those of the hot Am stars although there are definite similarities. Changes of up to order 1 dex are found by comparison with the previous analysis by Smith. Slightly better agreement is found with the recent analyses of singly-ionized rare earth lines by Magazzu and Cowley. Results are also presented for a model selected on the basis of photometric indices according to the formula of Moon and Dworetsky.
Adelman Saul J.
Bolcal Cetin
Inelmen Erol
Kocer Dursun
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