Abstract Two previous papers /1,2/ have shown that the dwarf nova OY Car has extensive vertical disc structure during its (∼2 week) superoutbursts. This structure is analogous to that seen in the low mass X-ray binaries (LMXBs), in that the whole disc flares towards its edge, and there is a bulge or “dark spot” where the mass transfer stream meets the disc edge. In this paper we present evidence that two more dwarf novae may have such a stream impact bulge, which manifests itself as a dip in the UV light curve, analogous to those seen in the X-ray light curves of the LMXB dippers.


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    Titel :

    The dwarf nova dippers


    Beteiligte:
    Naylor, T. (Autor:in) / Hassall, B.J.M. (Autor:in) / Charles, P.A. (Autor:in) / Sonneborn, G. (Autor:in)

    Erschienen in:

    Advances in Space Research ; 8 , 2-3 ; 321-324


    Erscheinungsdatum :

    1988-01-01


    Format / Umfang :

    4 pages




    Medientyp :

    Aufsatz (Zeitschrift)


    Format :

    Elektronische Ressource


    Sprache :

    Englisch



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