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2000MNRAS.316..647F - Mon. Not. R. Astron. Soc., 316, 647-656 (2000/August-2)
A model of slingshot prominences in rapidly rotating stars.
FERREIRA J.M.
Abstract (from CDS):
We discuss the question of what makes stellar prominences so different from their solar counterparts and what allows them to be detected. We also examine the role of the corotation radius in their formation.
Abstract Copyright: 2000, Royal Astronomical Society
Journal keyword(s): stars: activity - stars: coronae - stars: flare - stars: magnetic fields - stars: rotation 10.1046/j.1365-8711.2000.03544.x
Simbad objects: 3
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