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Autor:
Alexandr P. Antov, Margarita N. Lovkaya, Yury T. Tsap, Boris E. Zhilyaev, Oleg A. Svyatogorov, Volodymyr K. Taradii, Maxim V. Andreev, R. Bogdanovski, Alexandr V. Sergeev, B. Spassov, Renada Konstantinova-Antova, Arkadii V. Bondar, Irina A. Verlyuk, Kirill O. Stetsenko
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 436:1986-1992
V390 Aurigae is a rapidly rotating, chromospherically active late-type giant. The X-ray emission from the corona of V390 Aur, observed by the XMM–Newton space observatory, indicates intense flaring activity on this star. Multisite, coordinated high
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6c792a308baf83f76857ec5b1e7ccb7b
https://doi.org/10.1093/mnras/stt1706
https://doi.org/10.1093/mnras/stt1706
