Astronomy and Astrophysics – Astronomy
Scientific paper
Oct 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010apj...721.1034m&link_type=abstract
The Astrophysical Journal, Volume 721, Issue 2, pp. 1034-1043 (2010).
Astronomy and Astrophysics
Astronomy
1
Stars: Flare, Stars: Low-Mass, Stars: Magnetic Field
Scientific paper
Magnetic reconnection events in the atmospheres of low-mass dwarf stars can be classified as either slow or fast, depending on whether ohmic diffusion or Hall currents dominate in the reconnection process. We suggest that the separation of reconnection into slow and fast categories can help to explain some systematics of low-mass dwarfs as regards their emissions in X-rays, Hα, and radio. On the one hand, in the warmer dwarfs (
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