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EXOSAT observations of the Be/X-ray binaries 2S0114+65 and 4U2206+54

Published online by Cambridge University Press:  26 May 2016

Priyamvada Saraswat  and
Krishna M.V. Apparao
Priyamvada Saraswat
Affiliation:
Indian Institute of Astrophysics, Bangalore, India
Krishna M.V. Apparao
Affiliation:
Tata Institute of Fundamental Research, Bombay, India

Extract

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The X-ray source 2S0114+65 was identified as a Be star from its optical spectrum. The X-ray spectrum is hard and spectral fits indicate the presence of a large amount of circumstellar matter around the X-ray source. The source also undergoes transient X-ray outbursts as well as flaring activity is present. 2S0114+65 was observed with the EXOSAT satellite on four occasions: on 1983 July 28, 1985 December 29, 1986 January 1 and 2. We have carried out an analysis of the X-ray data on this star.

Type
3. X-Ray Observations
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 208 - 210
Copyright
Copyright © Kluwer 1994 

References

Saraswat, P. 1992, Ph.D. thesis and references therein Google Scholar
Apparao, K.M.V., Bisht, P., & Singh, K.P. 1991, ApJ 371, 772 Google Scholar
Saraswat, P. & Apparao, K.M.V. 1992, ApJ 401, 678 Google Scholar