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Pre-Main-Sequence Stellar Evolution

Published online by Cambridge University Press:  14 August 2015

G.S. Bisnovatyi-Kogan*
Affiliation:
Space Research Institute, Moscow, USSR

Abstract

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The problems of the stellar evolution to the main sequence are reviewed, taking into account the effects of mass loss, rotation and binarity. Properties of T Tauri stars are discussed which are connected with the recent observations of these stars in ultraviolet and X-ray regions. FU Ori phenomen is considered briefly.

Type
Session 2: Pre-Main-Sequence Evolution and Formation of Binary Stars
Copyright
Copyright © Reidel 1981 

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