Previous papers have shown that the dwarf nova OY Car has an extensive vertical disk structure during its superoutbursts. This structure is analogous to that seen in the low mass X-ray binaries (LMXBs), in that the whole disk flares toward its edge, and there is a bulge or 'dark spot' where the mass transfer stream meets the disk edge. The paper presents evidence suggesting 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:

    Erscheinungsdatum :

    1988-01-01



    Medientyp :

    Sonstige


    Format :

    Keine Angabe


    Sprache :

    Englisch


    Schlagwörter :


    The dwarf nova dippers

    Naylor, T. / Hassall, B.J.M. / Charles, P.A. et al. | Elsevier | 1988


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