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The X-ray history of WR 140 in modest comparison with the radio
Published online by Cambridge University Press: 25 May 2016
Abstract
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We present the X-ray lightcurve of the canonical colliding-wind binary WR 140 from the time of the last periastron through late 1997. Variations in column density, and intrinsic and absorbed X-ray flux agree well with the expectations of colliding wind theory in which the winds from the stars are spherically symmetric.
- Type
- Part 3. Interaction of Wolf-Rayet stars and other hot massive stars with their environment: colliding winds and ring nebulae
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- Copyright
- Copyright © Astronomical Society of the Pacific 1999
References
van der Hucht, K.A., Hidayat, B., (eds.) 1991, Wolf-Rayet Stars and Interrelations with Other Massive Stars in Galaxies, Proc. IAU Symp. No. 143 (Dordrecht: Kluwer)CrossRefGoogle Scholar
Pollock, A.M.T.
1998, in: Kaper, L. & Fullerton, A.W. (eds.), Cyclical Variability in Stellar Winds, Proc. ESO Workshop Garching Oct. 1997, ESO Ap. Symp. Ser. (Berlin: Springer), p. 110
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