Simple non-thermal models for the quiescent radio emission of dMe flare stars

Details Simple non-thermal models for the quiescent radio emission of dMe flare stars Simple non-thermal models for the quiescent radio emission of dMe flare stars

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...225..112w&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 225, no. 1, Nov. 1989, p. 112-124. Research supported by the Alexander von Hum

Astronomy and Astrophysics

Astronomy

38

Flare Stars, Late Stars, Radio Stars, Stellar Models, Synchrotron Radiation, Dwarf Stars, Radio Astronomy, Stellar Activity, Stellar Coronas, Stellar Magnetic Fields

Scientific paper

Simple nonthermal gyrosynchrotron models were applied to the quiescent emission of M dwarf stars. Evidence is presented which suggests that these stars have a number of smaller active regions contributing to the observed flux. The evidence includes an absence of Zeeman polarization in optical observations and a lack of polarization in quiescent emission.

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