Surface gravity and effective temperature of the K5 subdwarf G 224-58 A and Arcturus from the fits to Ti and MgH lines

We discuss here the results obtained in the determination of effective temperatures and metallicities of late-type stars. We provide the abundances of MgH, Ti ı and Ti װ, with a list of selected lines, for the red giant of Arcturus and the metal-poor K subdwarf G 224-58 A. The Sun was used as a temp...

Повний опис

Збережено в:
Бібліографічні деталі
Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2016
Автори: Kushniruk, I.O., Pavlenko, Ya.V., Gálvez-Ortiz, M.C., Zhang, Z.H.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2016
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/119944
Теги: Додати тег
Немає тегів, Будьте першим, хто поставить тег для цього запису!
Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Surface gravity and effective temperature of the K5 subdwarf G 224-58 A and Arcturus from the fits to Ti and MgH lines / I.O. Kushniruk, Ya.V. Pavlenko, M.C. Gálvez-Ortiz, Z.H. Zhang // Advances in Astronomy and Space Physics. — 2016. — Т. 6., вип. 1. — С. 16-19. — Бібліогр.: 18 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-119944
record_format dspace
spelling Kushniruk, I.O.
Pavlenko, Ya.V.
Gálvez-Ortiz, M.C.
Zhang, Z.H.
2017-06-10T13:12:29Z
2017-06-10T13:12:29Z
2016
Surface gravity and effective temperature of the K5 subdwarf G 224-58 A and Arcturus from the fits to Ti and MgH lines / I.O. Kushniruk, Ya.V. Pavlenko, M.C. Gálvez-Ortiz, Z.H. Zhang // Advances in Astronomy and Space Physics. — 2016. — Т. 6., вип. 1. — С. 16-19. — Бібліогр.: 18 назв. — англ.
2227-1481
DOI:10.17721/2227-1481.6.16-19
https://nasplib.isofts.kiev.ua/handle/123456789/119944
We discuss here the results obtained in the determination of effective temperatures and metallicities of late-type stars. We provide the abundances of MgH, Ti ı and Ti װ, with a list of selected lines, for the red giant of Arcturus and the metal-poor K subdwarf G 224-58 A. The Sun was used as a template star. After computing synthetic spectra for model atmospheres with different Teff and log g values, we used minimization procedures to determine the best fits to the observed features. The determination of Ti abundances was carried out in the framework of a self-consistent approach developed by Pavlenko et al. (2012). In the case of MgH we used similar minimization procedure. We present here the combination of two different approaches based on the fits performed to Ti and MgH, respectively. The resulting effective temperatures are Tₑff = 4300 K for Arcturus and Tₑff = 4600 K for G 224-58 A, where both solutions are degenerated with log g.
We thank Profs. Hinkle, Kurucz, and VALD3 team for providing databases of astrophysical data used in our work and anonymous Referee for some positive remarks.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
Surface gravity and effective temperature of the K5 subdwarf G 224-58 A and Arcturus from the fits to Ti and MgH lines
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Surface gravity and effective temperature of the K5 subdwarf G 224-58 A and Arcturus from the fits to Ti and MgH lines
spellingShingle Surface gravity and effective temperature of the K5 subdwarf G 224-58 A and Arcturus from the fits to Ti and MgH lines
Kushniruk, I.O.
Pavlenko, Ya.V.
Gálvez-Ortiz, M.C.
Zhang, Z.H.
title_short Surface gravity and effective temperature of the K5 subdwarf G 224-58 A and Arcturus from the fits to Ti and MgH lines
title_full Surface gravity and effective temperature of the K5 subdwarf G 224-58 A and Arcturus from the fits to Ti and MgH lines
title_fullStr Surface gravity and effective temperature of the K5 subdwarf G 224-58 A and Arcturus from the fits to Ti and MgH lines
title_full_unstemmed Surface gravity and effective temperature of the K5 subdwarf G 224-58 A and Arcturus from the fits to Ti and MgH lines
title_sort surface gravity and effective temperature of the k5 subdwarf g 224-58 a and arcturus from the fits to ti and mgh lines
author Kushniruk, I.O.
Pavlenko, Ya.V.
Gálvez-Ortiz, M.C.
Zhang, Z.H.
author_facet Kushniruk, I.O.
Pavlenko, Ya.V.
Gálvez-Ortiz, M.C.
Zhang, Z.H.
publishDate 2016
language English
container_title Advances in Astronomy and Space Physics
publisher Головна астрономічна обсерваторія НАН України
format Article
description We discuss here the results obtained in the determination of effective temperatures and metallicities of late-type stars. We provide the abundances of MgH, Ti ı and Ti װ, with a list of selected lines, for the red giant of Arcturus and the metal-poor K subdwarf G 224-58 A. The Sun was used as a template star. After computing synthetic spectra for model atmospheres with different Teff and log g values, we used minimization procedures to determine the best fits to the observed features. The determination of Ti abundances was carried out in the framework of a self-consistent approach developed by Pavlenko et al. (2012). In the case of MgH we used similar minimization procedure. We present here the combination of two different approaches based on the fits performed to Ti and MgH, respectively. The resulting effective temperatures are Tₑff = 4300 K for Arcturus and Tₑff = 4600 K for G 224-58 A, where both solutions are degenerated with log g.
issn 2227-1481
url https://nasplib.isofts.kiev.ua/handle/123456789/119944
citation_txt Surface gravity and effective temperature of the K5 subdwarf G 224-58 A and Arcturus from the fits to Ti and MgH lines / I.O. Kushniruk, Ya.V. Pavlenko, M.C. Gálvez-Ortiz, Z.H. Zhang // Advances in Astronomy and Space Physics. — 2016. — Т. 6., вип. 1. — С. 16-19. — Бібліогр.: 18 назв. — англ.
work_keys_str_mv AT kushnirukio surfacegravityandeffectivetemperatureofthek5subdwarfg22458aandarcturusfromthefitstotiandmghlines
AT pavlenkoyav surfacegravityandeffectivetemperatureofthek5subdwarfg22458aandarcturusfromthefitstotiandmghlines
AT galvezortizmc surfacegravityandeffectivetemperatureofthek5subdwarfg22458aandarcturusfromthefitstotiandmghlines
AT zhangzh surfacegravityandeffectivetemperatureofthek5subdwarfg22458aandarcturusfromthefitstotiandmghlines
first_indexed 2025-12-07T20:49:32Z
last_indexed 2025-12-07T20:49:32Z
_version_ 1850884041190932480