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T Tauri stars and flare stars: common properties and differences

Published online by Cambridge University Press:  23 September 2016

I. Appenzeller
I. Appenzeller*
Affiliation:
Landessternwarte Königstuhl D-6900 Heidelberg 1

Abstract

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T Tauri stars and flare stars are both magnetically active late-type stars of low mass and low to moderate luminosities. The flares observed in these two classes of variables show similar properties and, thus, probably have the same physical origin. On the other hand, at least the majority of the classical T Tauri stars seem to be surrounded by cool, dusty (accretion) disks, which are absent or undetectable in most classical flare stars.

Type
II Flare Stars and Related Objects T Tauri Stars
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 209 - 213
Copyright
Copyright © Kluwer 1990 

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