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2005A&A...433..323R - Astronomy and Astrophysics, volume 433, 323-334 (2005/4-1)
A simple model for the saturation of coronal X-ray emission of rapidly rotating late-type stars.
RYAN R.D., NEUKIRCH T. and JARDINE M.
Abstract (from CDS):
Abstract Copyright: ∼
Journal keyword(s): magnetohydrodynamics (MHD) - magnetic fields - stars: coronae - stars: late-type - stars: activity
Simbad objects: 1
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