Chemical abundances for A-and F-type supergiant stars
Abstract: We present the stellar parameters and elemental abundances of a set of A-F-type supergiant stars HD 45674, HD 180028, HD 194951 and HD 224893 using high resolution (R ≈ 42, 000) spectra taken from ELODIE library. We present the first results of the abundance analysis for HD 45674 and HD 224893. We reaffirm the abundances for HD 180028 and HD 194951 studied previously by Luck. Alpha-elements indicate that the objects belong to the thin disc population. Their abundances and their location on the Hertzsprung-Russell diagram seem to indicate that HD 45675, HD 194951 and HD 224893 are in the post-first dredge-up (post-1DUP) phase, and that they are moving in the red-blue loop region. HD 180028, on the contary, shows typical abundances of Population I, but its evolutionary status cannot be satisfactorily defined.
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Universidad Nacional Autónoma de México, Instituto de Astronomía
2016
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oai:scielo:S0185-110120160002003992018-05-17Chemical abundances for A-and F-type supergiant starsMolina,R. E.Rivera,H. stars: abundances stars: atmospheres stars: evolution super-giants Abstract: We present the stellar parameters and elemental abundances of a set of A-F-type supergiant stars HD 45674, HD 180028, HD 194951 and HD 224893 using high resolution (R ≈ 42, 000) spectra taken from ELODIE library. We present the first results of the abundance analysis for HD 45674 and HD 224893. We reaffirm the abundances for HD 180028 and HD 194951 studied previously by Luck. Alpha-elements indicate that the objects belong to the thin disc population. Their abundances and their location on the Hertzsprung-Russell diagram seem to indicate that HD 45675, HD 194951 and HD 224893 are in the post-first dredge-up (post-1DUP) phase, and that they are moving in the red-blue loop region. HD 180028, on the contary, shows typical abundances of Population I, but its evolutionary status cannot be satisfactorily defined.info:eu-repo/semantics/openAccessUniversidad Nacional Autónoma de México, Instituto de AstronomíaRevista mexicana de astronomía y astrofísica v.52 n.2 20162016-01-01info:eu-repo/semantics/articletext/htmlhttp://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012016000200399en |
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| author |
Molina,R. E. Rivera,H. |
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Molina,R. E. Rivera,H. Chemical abundances for A-and F-type supergiant stars |
| author_facet |
Molina,R. E. Rivera,H. |
| author_sort |
Molina,R. E. |
| title |
Chemical abundances for A-and F-type supergiant stars |
| title_short |
Chemical abundances for A-and F-type supergiant stars |
| title_full |
Chemical abundances for A-and F-type supergiant stars |
| title_fullStr |
Chemical abundances for A-and F-type supergiant stars |
| title_full_unstemmed |
Chemical abundances for A-and F-type supergiant stars |
| title_sort |
chemical abundances for a-and f-type supergiant stars |
| description |
Abstract: We present the stellar parameters and elemental abundances of a set of A-F-type supergiant stars HD 45674, HD 180028, HD 194951 and HD 224893 using high resolution (R ≈ 42, 000) spectra taken from ELODIE library. We present the first results of the abundance analysis for HD 45674 and HD 224893. We reaffirm the abundances for HD 180028 and HD 194951 studied previously by Luck. Alpha-elements indicate that the objects belong to the thin disc population. Their abundances and their location on the Hertzsprung-Russell diagram seem to indicate that HD 45675, HD 194951 and HD 224893 are in the post-first dredge-up (post-1DUP) phase, and that they are moving in the red-blue loop region. HD 180028, on the contary, shows typical abundances of Population I, but its evolutionary status cannot be satisfactorily defined. |
| publisher |
Universidad Nacional Autónoma de México, Instituto de Astronomía |
| publishDate |
2016 |
| url |
http://www.scielo.org.mx/scielo.php?script=sci_arttext&pid=S0185-11012016000200399 |
| work_keys_str_mv |
AT molinare chemicalabundancesforaandftypesupergiantstars AT riverah chemicalabundancesforaandftypesupergiantstars |
| _version_ |
1756220874038444032 |