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Интеллектуальная Система Тематического Исследования НАукометрических данных |
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Parametrization of long-period eclipsing binariesтезисы доклада
- Авторы: Pakhomova P., Berdnikov L., Kniazev A., Katkov I., Malkov O.
- Сборник: ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES
- Серия: Proceedings of the VAK-2021 conference, Aug 23–28, 2021 (Edited by A.M. Cherepashchuk et al.)
- Тезисы
- Глава в коллективной монографии
- Год издания: 2022
- Место издания: Janus-K Москва
- Первая страница: 460
- Последняя страница: 462
- DOI: 10.51194/VAK2021.2022.1.1.192
- Аннотация: One of the important sources for independent determination of stellar masses are eclipsing binaries with components on theMain Sequence, and with observable spectral lines of both components. The parameters of such stars are used to constructthe mass-luminosity relation for stars of high and intermediate masses. Among them, the type of long-period eclipsingbinaries stands out, the parameters of which are currently not fully determined, which is associated with the difficultiescaused by the need for long-term observations. In this article we will review the currently available observational data forsuch objects and discuss the prospects for their use to determine stellar masses.
- Добавил в систему: Бердников Леонид Николаевич