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Autor:
A. V. Bondar, O. A. Svyatogorov, V. N. Petukhov, B. E. Zhilyaev, I. A. Verlyuk, S. M. Pokhvala, Yu. M. Ivashchenko, V. M. Reshetnyk, M. V. Andreev
Publikováno v:
Kinematics and Physics of Celestial Bodies. 31:267-275
We report on the detection of rapid variability in subsecond mode in the Balmer lines of hydrogen, lines Ca II H,K, and b Mg I triplet in chromospherically active stars 61 Cyg A, B. The spectral observations of 61 Cyg A, B were performed with MMCS sp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::6a7bb44fbf7d1de4149177a7ecf450a2
https://doi.org/10.3103/s0884591315060082
https://doi.org/10.3103/s0884591315060082
