A simple model for the saturation of coronal X-ray emission of rapidly rotating late-type stars

Publisher: Edp Sciences

E-ISSN: 1432-0746|433|1|323-334

ISSN: 0004-6361

Source: Astronomy & Astrophysics, Vol.433, Iss.1, 2005-04, pp. : 323-334

Disclaimer: Any content in publications that violate the sovereignty, the constitution or regulations of the PRC is not accepted or approved by CNPIEC.

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