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...

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Бібліографічні деталі
Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2013
Автори: Kushniruk, I.O., Pavlenko, Ya.V., Kaminskiy, B.M.
Формат: Стаття
Мова:Англійська
Опубліковано: Головна астрономічна обсерваторія НАН України 2013
Онлайн доступ:https://nasplib.isofts.kiev.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.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Kushniruk, I.O.
Pavlenko, Ya.V.
Kaminskiy, B.M.
author_facet Kushniruk, I.O.
Pavlenko, Ya.V.
Kaminskiy, B.M.
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.
collection DSpace DC
container_title Advances in Astronomy and Space Physics
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.
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last_indexed 2025-12-07T21:09:26Z
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publisher Головна астрономічна обсерваторія НАН України
record_format dspace
spelling Kushniruk, I.O.
Pavlenko, Ya.V.
Kaminskiy, B.M.
2017-06-06T19:04:32Z
2017-06-06T19:04:32Z
2013
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
https://nasplib.isofts.kiev.ua/handle/123456789/119418
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.
We thank to Profs. Hinkle, Kurucz, and VALD team for providing databases of astrophysical data used in our work, Oleksiy Ivanyuk and Larisa Yakovina for the helpful comments, and anonymous Referee for some positive remarks.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
MgH lines in the spectrum of Arcturus
Article
published earlier
spellingShingle MgH lines in the spectrum of Arcturus
Kushniruk, I.O.
Pavlenko, Ya.V.
Kaminskiy, B.M.
title 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_short MgH lines in the spectrum of Arcturus
title_sort mgh lines in the spectrum of arcturus
url https://nasplib.isofts.kiev.ua/handle/123456789/119418
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AT pavlenkoyav mghlinesinthespectrumofarcturus
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