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The statistical analysis of the optical and infrared luminosities of young stars

Published online by Cambridge University Press:  23 September 2016

T.A. Movsessian
T.A. Movsessian*
Affiliation:
Byurakan Astrophysical Observatory Armenian Academy of Sciences, USSR

Abstract

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The infrared IRAS data for supposed sources of optical outflows and young stars in Taurus-Auriga complex are studied. It is shown that there exists a group of stars with extremely low optical and infrared luminosities. It's suggested, that they are the stars with anisotropic sourface activity.

Type
III Flare Stars and Related Objects Fuors and Other Non-Stable Objects
Information
Symposium - International Astronomical Union , Volume 137: Flare Stars in Star Clusters, Association and Solar Vicinity , 1990 , pp. 283 - 286
Copyright
Copyright © Kluwer 1990 

References

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