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Optical and J, K-photometry of the quiescent black hole X-ray nova A0620-00 in the passive and active statesстатья
Статья опубликована в высокорейтинговом журнале
Информация о цитировании статьи получена из
Web of Science
Статья опубликована в журнале из списка Web of Science и/или Scopus
Дата последнего поиска статьи во внешних источниках: 21 мая 2019 г.
- Авторы: Cherepashchuk A.M., Katysheva N.A., Khruzina T.S., Shugarov S.Y., Tatarnikov A.M., Burlak M.A., Shatsky N.I.
- Журнал: Monthly Notices of the Royal Astronomical Society
- Том: 483
- Номер: 2
- Год издания: 2019
- Издательство: Oxford Journals, Oxford University Press
- Местоположение издательства: Oxford, UK, England
- Первая страница: 1067
- Последняя страница: 1079
- DOI: 10.1093/mnras/sty3166
- Аннотация: In 2015–2016, the X-ray nova A0620−00 in quiescence was observed in the passive state, according to the terminology of Cantrell et al., and in less than 230 d it transited into the active state. The system mean luminosity increased by 0.20 mag in the optical and by 0.25 and 0.30 mag in J and K infrared bands, respectively, while the orbital light curves changed drastically, and the flickering amplitude more than doubled. The mean light-curve analysis performed in the context of two models argued that the interaction region where the gas stream reaches the disc is responsible for these effects. The growth of this region’s luminosity in the active state implies the increase of the mass transfer rate via the L1 point, likely due to non-stationary processes in the donor star atmosphere. The non-stellar spectrum Fλ in the observed range λλ6400--22000 Å obeys a power law of λα where α = −(2.13 ± 0.1) in the passive state and α = −(1.85 ± 0.1) in the active, while the absolute mean square flickering amplitude behaves like ΔFfl(λ) ∼ λ−2.36 in both states of activity.
- Добавил в систему: Шугаров Сергей Юрьевич
Прикрепленные файлы
| № | Имя | Описание | Имя файла | Размер | Добавлен |
|---|---|---|---|---|---|
| 1. | Полный текст | mn483-1067.pdf | 2,1 МБ | 6 февраля 2019 [s_shugarov] |