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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
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 © Astronomical Society of the Pacific 1999