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.


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    Titel :

    X-ray variability in V444 Cygni — Evidence for colliding winds


    Beteiligte:
    Corcoran, M.F. (Autor:in) / Shore, S.N. (Autor:in) / Swank, J.H. (Autor:in) / Heap, S.R. (Autor:in) / Rawley, G.L. (Autor:in) / Pollock, A.M.T. (Autor:in) / Stevens, I.R. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 13 , 12 ; 295-297


    Erscheinungsdatum :

    1993-01-01


    Format / Umfang :

    3 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



    X-ray variability in V444 Cygni-Evidence for colliding winds

    Corcoran, M. F. / Shore, S. N. / Swank, J. H. et al. | NTRS | 1993


    X-Ray Variability in V444 Cygni - Evidence for Colliding Winds

    Corcoran, M. F. / Shore, S. N. / Swank, J. H. et al. | British Library Conference Proceedings | 1993



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