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X-ray astronomy of stellar coronae
DOI: 10.1007/s00159-004-0023-2 Bibcode: 2004A&ARv..12...71G

Güdel, Manuel

X-ray emission from stars in the cool half of the Hertzsprung-Russell diagram is generally attributed to the presence of a magnetic corona that contains plasma at temperatures exceeding 1 million K. Coronae are ubiquitous among these stars, yet many fundamental mechanisms operating in their magnetic fields still elude an interpretation through a d…

2004 Astronomy and Astrophysics Review
XMM-Newton 406