Magnetic stars with wide depressions in the continuum. 2. The silicon star with a complex field structure HD 27404
- Авторлар: Semenko E.A.1, Romanyuk I.I.1, Semenova E.S.2, Moiseeva A.V.1, Kudryavtsev D.O.1, Yakunin I.A.1
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Мекемелер:
- Special Astrophysical Observatory
- Kazan (Volga region) Federal University
- Шығарылым: Том 72, № 4 (2017)
- Беттер: 384-390
- Бөлім: Article
- URL: https://journals.rcsi.science/1990-3413/article/view/212542
- DOI: https://doi.org/10.1134/S1990341317040034
- ID: 212542
Дәйексөз келтіру
Аннотация
Observations of the chemically peculiar star HD 27404 with the 6-m SAO RAS telescope showed a strong magnetic field with the longitudinal field component varying in a complicated way in the range of −2.5 to 1 kG. Fundamental parameters of the star (Teff = 11 300 K, log g = 3.9) were estimated analyzing photometric indices in the Geneva and in the Stro¨ mgren–Crawford photometric systems. We detected weak radial velocity variations which can be due to the presence of a close star companion or chemical spots in the photosphere. Rapid estimation of the key chemical element abundance allows us to refer HD 27404 to a SiCr or Si+ chemically peculiar A0–B9 star.
Негізгі сөздер
Авторлар туралы
E. Semenko
Special Astrophysical Observatory
Хат алмасуға жауапты Автор.
Email: sea@sao.ru
Ресей, Nizhnii Arkhyz, 369167
I. Romanyuk
Special Astrophysical Observatory
Email: sea@sao.ru
Ресей, Nizhnii Arkhyz, 369167
E. Semenova
Kazan (Volga region) Federal University
Email: sea@sao.ru
Ресей, Kazan, 420008
A. Moiseeva
Special Astrophysical Observatory
Email: sea@sao.ru
Ресей, Nizhnii Arkhyz, 369167
D. Kudryavtsev
Special Astrophysical Observatory
Email: sea@sao.ru
Ресей, Nizhnii Arkhyz, 369167
I. Yakunin
Special Astrophysical Observatory
Email: sea@sao.ru
Ресей, Nizhnii Arkhyz, 369167
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