Пожалуйста, используйте этот идентификатор, чтобы цитировать или ссылаться на этот ресурс: http://elar.urfu.ru/handle/10995/131041
Название: Characteristics of Long-Term Spot Activity on Several Late-Spectral-Type Stars
Авторы: Kozhevnikova, A. V.
Alekseev, I. Y.
Kozhevnikov, V. P.
Дата публикации: 2023
Издатель: Pleiades Publishing
Библиографическое описание: Kozhevnikova, A, Alekseev, I & Kozhevnikov, V 2023, 'Characteristics of Long-Term Spot Activity on Several Late-Spectral-Type Stars', Astronomy Reports, Том. 67, № 9, стр. 929-937. https://doi.org/10.1134/S1063772923090081
Kozhevnikova, A., Alekseev, I., & Kozhevnikov, V. (2023). Characteristics of Long-Term Spot Activity on Several Late-Spectral-Type Stars. Astronomy Reports, 67(9), 929-937. https://doi.org/10.1134/S1063772923090081
Аннотация: Abstract: We present our analysis of many-year photometry for several dozens of chromospherically active stars that exhibit solar-type activity (from our own observations as well as from data in the literature). Modeling of the distribution of cool photospheric spots, based on the zonal model, was performed, with several hundred models constructed. We find that, for most stars, their spots are located at intermediate and moderate latitudes and that the largest spotted areas can cover from 7 to 58% of the star’s surface. We demonstrate that a latitude drift of spots can be suspected for a number of stars, towards the equator as well as towards the pole; however, the rate of this drift is several times lower than for solar spots. For 15 stars, we detected the presence of activity cycles from 3 to 28 years long that reveal themselves in variations of the system’s brightness as well as in variations of the total spot coverage of the star. This paper is based on a talk presented at the memorial astrophysical workshop “Novelties in Understanding the Evolution of Binary Stars” dedicated to the 90th birthday of Prof. M.A. Svechnikov. © 2023, The Author(s).
Ключевые слова: STAR SPOTS
STELLAR ACTIVITY
VARIABLE STARS
URI: http://elar.urfu.ru/handle/10995/131041
Условия доступа: info:eu-repo/semantics/openAccess
cc-by
Текст лицензии: https://creativecommons.org/licenses/by/4.0/
Идентификатор РИНЦ: 64456380
Идентификатор SCOPUS: 85179351529
Идентификатор WOS: 001122207000002
Идентификатор PURE: 49822557
ISSN: 1063-7729
DOI: 10.1134/S1063772923090081
Сведения о поддержке: Ministry of Education and Science of the Russian Federation, Minobrnauka: FEUZ-2023-0019
Thus study was financially supported by the Ministry of Science and Higher Education of Russian Federation, theme FEUZ-2023-0019.
Располагается в коллекциях:Научные публикации ученых УрФУ, проиндексированные в SCOPUS и WoS CC

Файлы этого ресурса:
Файл Описание РазмерФормат 
2-s2.0-85179351529.pdf955,94 kBAdobe PDFПросмотреть/Открыть


Лицензия на ресурс: Лицензия Creative Commons Creative Commons