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pro vyhledávání: '"Reiners, D. Shulyak A."'
Publikováno v:
Nature Astronomy, Volume 1, id. 0184 (2017)
M dwarfs are the most numerous stars in our Galaxy with masses between approximately 0.5 and 0.1 solar mass. Many of them show surface activity qualitatively similar to our Sun and generate flares, high X-ray fluxes, and large-scale magnetic fields.
Externí odkaz:
http://arxiv.org/abs/1801.08571