MgH lines in the spectrum of Arcturus
The synthetic spectra of MgH lines were computed for the grid of the model atmospheres and compared with the observed spectrum of Arcturus. The parameters of the atmosphere of Arcturus for log g = 1.5 and Tₑff = 4300K were via minimization of deviation between observed and computed spectra and compa...
Збережено в:
| Дата: | 2013 |
|---|---|
| Автори: | , , |
| Формат: | Стаття |
| Мова: | English |
| Опубліковано: |
Головна астрономічна обсерваторія НАН України
2013
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| Назва видання: | Advances in Astronomy and Space Physics |
| Онлайн доступ: | http://dspace.nbuv.gov.ua/handle/123456789/119418 |
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| Назва журналу: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Цитувати: | MgH lines in the spectrum of Arcturus / I.O. Kushniruk, Ya.V. Pavlenko, B.M. Kaminskiy // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 29-31. — Бібліогр.: 12 назв. — англ. |
Репозитарії
Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
irk-123456789-119418 |
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| record_format |
dspace |
| spelling |
irk-123456789-1194182017-06-07T03:02:29Z MgH lines in the spectrum of Arcturus Kushniruk, I.O. Pavlenko, Ya.V. Kaminskiy, B.M. The synthetic spectra of MgH lines were computed for the grid of the model atmospheres and compared with the observed spectrum of Arcturus. The parameters of the atmosphere of Arcturus for log g = 1.5 and Tₑff = 4300K were via minimization of deviation between observed and computed spectra and compared with the results of other studies. 2013 Article MgH lines in the spectrum of Arcturus / I.O. Kushniruk, Ya.V. Pavlenko, B.M. Kaminskiy // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 29-31. — Бібліогр.: 12 назв. — англ. 2227-1481 http://dspace.nbuv.gov.ua/handle/123456789/119418 en Advances in Astronomy and Space Physics Головна астрономічна обсерваторія НАН України |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| language |
English |
| description |
The synthetic spectra of MgH lines were computed for the grid of the model atmospheres and compared with the observed spectrum of Arcturus. The parameters of the atmosphere of Arcturus for log g = 1.5 and Tₑff = 4300K were via minimization of deviation between observed and computed spectra and compared with the results of other studies. |
| format |
Article |
| author |
Kushniruk, I.O. Pavlenko, Ya.V. Kaminskiy, B.M. |
| spellingShingle |
Kushniruk, I.O. Pavlenko, Ya.V. Kaminskiy, B.M. MgH lines in the spectrum of Arcturus Advances in Astronomy and Space Physics |
| author_facet |
Kushniruk, I.O. Pavlenko, Ya.V. Kaminskiy, B.M. |
| author_sort |
Kushniruk, I.O. |
| title |
MgH lines in the spectrum of Arcturus |
| title_short |
MgH lines in the spectrum of Arcturus |
| title_full |
MgH lines in the spectrum of Arcturus |
| title_fullStr |
MgH lines in the spectrum of Arcturus |
| title_full_unstemmed |
MgH lines in the spectrum of Arcturus |
| title_sort |
mgh lines in the spectrum of arcturus |
| publisher |
Головна астрономічна обсерваторія НАН України |
| publishDate |
2013 |
| url |
http://dspace.nbuv.gov.ua/handle/123456789/119418 |
| citation_txt |
MgH lines in the spectrum of Arcturus / I.O. Kushniruk, Ya.V. Pavlenko, B.M. Kaminskiy // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 29-31. — Бібліогр.: 12 назв. — англ. |
| series |
Advances in Astronomy and Space Physics |
| work_keys_str_mv |
AT kushnirukio mghlinesinthespectrumofarcturus AT pavlenkoyav mghlinesinthespectrumofarcturus AT kaminskiybm mghlinesinthespectrumofarcturus |
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2023-10-18T20:34:31Z |
| last_indexed |
2023-10-18T20:34:31Z |
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1796150558156914688 |