Cool Spots on the Surface of the Active Giant PZ Mon
- Авторы: Pakhomov Y.V.1, Shenavrin V.I.2, Bondar’ N.I.3, Antonyuk K.A.3, Pit’ N.V.3, Belan S.P.3, Gorda S.Y.4
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Учреждения:
- Institute of Astronomy
- Sternberg Astronomical Institute
- Crimean Astrophysical Observatory
- Kourovka Astronomical Observatory
- Выпуск: Том 45, № 3 (2019)
- Страницы: 156-163
- Раздел: Article
- URL: https://ogarev-online.ru/1063-7737/article/view/191141
- DOI: https://doi.org/10.1134/S1063773719030058
- ID: 191141
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Аннотация
Based on the multicolor (BVRIJHKL) photometric observations of the active red giant PZ Mon performed for the first time in the winter season of 2017–2018, we have determined the main characteristics of the spotted stellar surface in a parametric three-spot model. The unspotted surface temperature is Teff = 4730 K, the temperature of the cool spots is Ts = 3500 K, their relative area is about 41%, and the temperature of the warm spots is ∼4500 K with a maximum relative area up to 20%.The distribution of spots over the stellar surface has been modeled. The warm spots have been found to be distributed at various longitudes in the hemisphere on the side of the secondary component and are most likely a result of its influence.
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Об авторах
Yu. Pakhomov
Institute of Astronomy
Автор, ответственный за переписку.
Email: pakhomov@inasan.ru
Россия, Pyatnitskaya ul. 48, Moscow, 109017
V. Shenavrin
Sternberg Astronomical Institute
Email: pakhomov@inasan.ru
Россия, Universitetskii pr. 13, Moscow, 119992
N. Bondar’
Crimean Astrophysical Observatory
Email: pakhomov@inasan.ru
Россия, Nauchny, Crimea, 298409
K. Antonyuk
Crimean Astrophysical Observatory
Email: pakhomov@inasan.ru
Россия, Nauchny, Crimea, 298409
N. Pit’
Crimean Astrophysical Observatory
Email: pakhomov@inasan.ru
Россия, Nauchny, Crimea, 298409
S. Belan
Crimean Astrophysical Observatory
Email: pakhomov@inasan.ru
Россия, Nauchny, Crimea, 298409
S. Gorda
Kourovka Astronomical Observatory
Email: pakhomov@inasan.ru
Россия, ul. Mira 19, Yekaterinburg, 620002
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