Radio emission from stellar flares

Details Radio emission from stellar flares Radio emission from stellar flares

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989soph..121..163k&link_type=abstract

(IAU, Colloquium on Solar and Stellar Flares, 104th, Stanford, CA, Aug. 15-19, 1988) Solar Physics (ISSN 0038-0938), vol. 121, n

Physics

21

Coherent Electromagnetic Radiation, Radio Emission, Stellar Flares, Accretion Disks, Binary Stars, Early Stars, X Ray Binaries

Scientific paper

An overview is given of the observations of stellar radio 'flares', defined as radio emission which is both variable in time and created by explosive releases of magnetic energy. The main sources of such flares are late-type main-sequence stars, classic close binaries, X-ray binaries, and premain-sequence stars. The interpretations of these observations in terms of the various incoherent and coherent emission mechanisms are summarized. The possible importance of a coherent emission process in electrostatic double layers is pointed out. The diagnostic importance of radio emission for the flare process in classic and compact stars is briefly described. In particular, the possible production of radio flares from interactions between an accretion disk and the magnetic field of the central object is discussed.

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