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Prospects for studies of UV Cet-type flare stars

Published online by Cambridge University Press:  23 September 2016

M. Rodono'
M. Rodono'*
Affiliation:
Astronomy Institute of Catania University, and Catania Astrophysical Observatory Viale A. Doria 6 I-95125 Catania Italy

Abstract

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The present review addresses selected questions on UV Cet-type red-dwarf stars primarily concerning the physics involved in the various aspects and phases of the flare phenomenon, rather than the average activity behaviour of the flare stars. In fact, while flare activity level and general trend are reasonably well established, a fully consistent physical picture of both solar and stellar flare events is still missing. Some recent results are presented with the aim of showing which observations are needed and the relevant role that coordinated multiband studies can play.

Type
V Prospects for Stellar Flare Research and Concluding Remarks
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 371 - 391
Copyright
Copyright © Kluwer 1990 

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