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Ultraviolet Observations of Close Binary Stars

Published online by Cambridge University Press:  14 August 2015

R. S. Polidan  and
G. J. Peters
R. S. Polidan
Affiliation:
Princeton University Observatory Princeton, NJ 08540 USA
G. J. Peters
Affiliation:
Department of Astronomy University of Southern California Los Angeles, CA 90007 USA

Abstract

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In this paper, we present far ultraviolet observations of three interacting binary stars (HR 2142, HR 7084, and λ Tauri). All stars exhibit evidence of a gas stream and extensive mass outflow from the system. Physical parameters are derived for the gas stream in HR 2142.

Type
V. Algol and Algols
Information
Symposium - International Astronomical Union , Volume 88: Close Binary Stars: Observations and Interpretation , 1980 , pp. 293 - 297
Copyright
Copyright © Reidel 1980 

References

Koubsky, P.: 1978, Bull. Astron. Inst. Czechosl., 29, pp. 288.Google Scholar
Lubow, S. and Shu, F.: 1975, Astroph. J., 198, pp. 383.CrossRefGoogle Scholar
Peters, G. J.: 1976, in Be and Shell Stars (Ed. Slettebak, A.), IAU Symp. No. 70, pp. 417.Google Scholar
Peters, G. J. and Polidan, R. S.: 1973, in Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems, IAU Symp. No. 51, pp. 174.Google Scholar
Rogerson, J. B., Spitzer, L., Drake, J. F., Dressler, K., Jenkins, E., Morton, D. C., and York, D. G.: 1973, Astroph. J., 181, pp. L97.CrossRefGoogle Scholar