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Radio emission from stellar flares

  • Solar and Stellar Flares
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Abstract

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 pre-Main-Sequence stars.

We summarize the interpretations of these observations in terms of the various incoherent and coherent emission mechanisms. The possible importance of a coherent emission process in electrostatic double layers is pointed out.

We briefly indicate the diagnostic importance of radio emission for the flare process in classic and compact stars. In particular we discuss the possible production of radio flares from interactions between an accretion disk and the magnetic field of the central object.

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  1. Sterrkundig Instituut, Utrecht University, P.O. Box 80000, 3508 TA, Utrecht, The Netherlands

    Jan Kuijpers

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Kuijpers, J. Radio emission from stellar flares. Sol Phys 121, 163–185 (1989). https://doi.org/10.1007/BF00161694

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