Abstract Phase-resolved ROSAT observations of the soft X-ray flux from V444 Cygni confirm the orbital dependence of the flux suggested by analysis of 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 ; 295-297
1993-01-01
3 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
X-Ray Variability in V444 Cygni - Evidence for Colliding Winds
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