Phase-resolved ROSAT observations of the soft X-ray flux from V444 Cygni confirm the orbital dependence of the flux suggested by analysis of imaging proportional counter (IPC) observations. The X-ray behavior suggests that a region of X-ray emitting gas exists between the 2 stars, probably produced by a collision between the WR and O star winds.
X-ray variability in V444 Cygni-Evidence for colliding winds
Advances in Space Research ; 13 , 12
1993-12-01
Miscellaneous
No indication
English
X-Ray Variability in V444 Cygni - Evidence for Colliding Winds
British Library Conference Proceedings | 1993
|X-ray variability in V444 Cygni — Evidence for colliding winds
Elsevier | 1993
|X-Ray Variability in V444 Cygni - Evidence for Colliding Winds
Online Contents | 1993
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Online Contents | 1998
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