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Ultraviolet Observations, Stellar Winds, and Mass Loss for Be Stars

Published online by Cambridge University Press:  14 August 2015

J. M. Marlborough
J. M. Marlborough*
Affiliation:
Astronomy Centre, The University of Sussex, Falmer, U.K. Department of Astronomy, The University of Western Ontario, London, Ontario, Canada

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Although the first ultraviolet (UV) observation of an astronomical source was obtained in 1946, the first UV observations of Be stars were not obtained until 1964. In this review of UV data covering the period since 1964, the term Be star will be assumed to include Oe stars as well (Frost and Conti, 1976). An earlier review of this subject is by Heap (1976).

Type
VII. UV Observations and Mass Loss
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 361 - 376
Copyright
Copyright © Reidel 1982 

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