The May 1985 superoutburst of OY Carinae: I. Structure of the outer disk from optical and IR observations

T. Naylor*, J. Bailey, F. M. Bateson, G. Berriman, P. A. Charles, I. M. Coulson, A. R. Hyland, K. Reinsch, B. Warner, P. A. Whitelock

*Corresponding author for this work

    Research output: Contribution to journalArticlepeer-review

    Abstract

    We present optical and IR observations of the dwarf nova OY Car during the May 1985 superoutburst. From them we find that the superhump has a temperature of ∼8000K and an area of order half the size of the red dwarf or accretion disk. We also compare the behaviour during two simultaneous optical/IR observations. Whilst the light curves in the two pass bands are similar during one observation, in the other observation they show marked differences that may be due to a cool region in the outer disk.

    Original languageEnglish
    Pages (from-to)365-369
    Number of pages5
    JournalAstrophysics and Space Science
    Volume130
    Issue number1-2
    DOIs
    Publication statusPublished - Feb 1987

    Fingerprint

    Dive into the research topics of 'The May 1985 superoutburst of OY Carinae: I. Structure of the outer disk from optical and IR observations'. Together they form a unique fingerprint.

    Cite this