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Recent Changes in the Ultraviolet Spectrum of the Be Star HR 2855

Published online by Cambridge University Press:  14 August 2015

Geraldine J. Peters
Geraldine J. Peters*
Affiliation:
Department of Astronomy, University of Southern California, Los Angeles, CA 90007 USA

Extract

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High resolution IUE observations of the Be star HR 2855 (HD 58978) spaced five months apart have revealed striking variations in the resonance lines of C IV and N V. The nature of these variations can be seen in Figures 1 and 2.

Type
VII. UV Observations and Mass Loss
Information
Symposium - International Astronomical Union , Volume 98: Be Stars , 1982 , pp. 411 - 414
Copyright
Copyright © Reidel 1982 

References

Doazan, V., Kuhi, L.V., Thomas, R.N.: 1980, Astrophys. J. 235, pp. L17–L20.Google Scholar
Doazan, V., Grady, C., Kuhi, L.V., Marlborough, J.M., Snow, T.P., and Thomas, R.N.: 1982, this volume, pp. 415–418.Google Scholar
Hubert-Delplace, A.M. and Hubert, H.: 1979, An Atlas of Be Stars, Observatoire de Meudori, France.Google Scholar