The Structure of the Corona of dMe Flare Stars

Details The Structure of the Corona of dMe Flare Stars The Structure of the Corona of dMe Flare Stars

May 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992aas...180.6005w&link_type=abstract

American Astronomical Society, 180th AAS Meeting, #60.05; Bulletin of the American Astronomical Society, Vol. 24, p.826

Astronomy and Astrophysics

Astronomy

Scientific paper

There is now considerable information on both the surface magnetic fields of dMe flare stars and on the thermal (X-ray emitting) populations in their coronae. We show that the simplest picture of the corona of a dMe flare star based on the measured photospheric magnetic field strengths, the measured filling factors of these fields, and the X-ray emission from their coronae, are inconsistent with radio observations of the coronae. We discuss possible resolutions of this dilemma.

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