Features of magnetic field structures in chemically peculiar stars. IV
- Авторлар: Glagolevskij Y.V.1, Nazarenko A.F.1
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Мекемелер:
- Special Astrophysical Observatory
- Шығарылым: Том 71, № 4 (2016)
- Беттер: 453-462
- Бөлім: Article
- URL: https://journal-vniispk.ru/1990-3413/article/view/212306
- DOI: https://doi.org/10.1134/S1990341316040088
- ID: 212306
Дәйексөз келтіру
Аннотация
We present results of modeling of the sample of magnetic stars. We have obtained such important for magnetic star physics parameters as the mean surface magnetic field Bs, the magnetic field at magnetic poles—Bp, the dipole inclination to the rotation equatorial plane α, and the distance to monopoles from the center of the star Δa. We present some information onmagnetic star physics that helps to understand the derived results better.
Негізгі сөздер
Авторлар туралы
Yu. Glagolevskij
Special Astrophysical Observatory
Хат алмасуға жауапты Автор.
Email: glagol@sao.ru
Ресей, Nizhnii Arkhyz, 369167
A. Nazarenko
Special Astrophysical Observatory
Email: glagol@sao.ru
Ресей, Nizhnii Arkhyz, 369167
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