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Flare activity of stars in the Taurus region

Published online by Cambridge University Press:  23 September 2016

A.S. Hojaev
A.S. Hojaev*
Affiliation:
High Energy Astrophisics Department Astronomical Institute Uzbek Academy of Sciences, USSR

Abstract

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Using the actual observational data on photometric and spectral stellar activity in the region of central area of the Taurus Dark Clouds complex, the question of flare activity of the stars and its connection with another kinds of activities is considered. The comparison of stellar flares in this region with that of in other associations and clusters (especially, Orion and Pleiades) is made and the youth of the group in Taurus is shown. The detection of flaring variables (including stars with T Tauri-type features) in Taurus region is the evidence in favour of evolutionary connection of these stages.

Type
I Flare Stars Optical Observations and Flare Statistics
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 81 - 84
Copyright
Copyright © Kluwer 1990 

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