NLTE CALCULATION FOR O II
The Kurucz's atmospheric models and a modified version of the MULTI code are applied in a NLTE investigation of the O II spectrum. It is shown that previously performed analyses based on the use of lightly line- blanketed Gold models give results that are in variance with those based on the use...
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Odessa I. I. Mechnykov National University
2017-03-01
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doaj-e79e1157bbdd41fd9f5f55d99e8cad782020-11-25T02:48:36ZengOdessa I. I. Mechnykov National UniversityOdessa Astronomical Publications1810-42152017-03-0112019119410.18524/1810-4215.1999.12.9303193031NLTE CALCULATION FOR O IIS. A. Korotin0Astronomical Observatory, Odessa State University, T.G.Shevchenko Park, Odessa 65014 UkraineThe Kurucz's atmospheric models and a modified version of the MULTI code are applied in a NLTE investigation of the O II spectrum. It is shown that previously performed analyses based on the use of lightly line- blanketed Gold models give results that are in variance with those based on the use of the more heavily blanketed Kurucz's models. One result of our calculations is a number of useful relationships between the NLTE oxygen abundance, line equivalent width, and stellar atmospheric parameters.http://oap.onu.edu.ua/article/view/93031 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
S. A. Korotin |
spellingShingle |
S. A. Korotin NLTE CALCULATION FOR O II Odessa Astronomical Publications |
author_facet |
S. A. Korotin |
author_sort |
S. A. Korotin |
title |
NLTE CALCULATION FOR O II |
title_short |
NLTE CALCULATION FOR O II |
title_full |
NLTE CALCULATION FOR O II |
title_fullStr |
NLTE CALCULATION FOR O II |
title_full_unstemmed |
NLTE CALCULATION FOR O II |
title_sort |
nlte calculation for o ii |
publisher |
Odessa I. I. Mechnykov National University |
series |
Odessa Astronomical Publications |
issn |
1810-4215 |
publishDate |
2017-03-01 |
description |
The Kurucz's atmospheric models and a modified version of the MULTI code are applied in a NLTE investigation of the O II spectrum. It is shown that previously performed analyses based on the use of lightly line- blanketed Gold models give results that are in variance with those based on the use of the more heavily blanketed Kurucz's models. One result of our calculations is a number of useful relationships between the NLTE oxygen abundance, line equivalent width, and stellar atmospheric parameters. |
url |
http://oap.onu.edu.ua/article/view/93031 |
work_keys_str_mv |
AT sakorotin nltecalculationforoii |
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1724747588164386816 |