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T Tauri and FU Orionis Stars

Published online by Cambridge University Press:  14 August 2015

G. F. Gahm
G. F. Gahm*
Affiliation:
Stockholm Observatory, Saltsjöbaden, Sweden

Abstract

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A great deal of information on the continuous radiation of T Tau- and similar type stars has been acquired. The cause of the ultraviolet and infrared excess emission is discussed. The possibility that the blue continuum may arise from numerous line emissions is considered. Various possibilities for the cause of the light variations are described, as well as the nature of the emission lines. The special features of the FU Ori stars are mentioned.

Type
Part 1 / Flare Stars and T Tauri Stars
Information
Symposium - International Astronomical Union , Volume 67: Variable Stars and Stellar Evolution , 1975 , pp. 101 - 107
Copyright
Copyright © Reidel 1975 

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