A search for 843 MHz radio emission from active stars

Alan Vaughan, M. I. Large

    Research output: Contribution to journalArticlepeer-review


    Known Southern flare stars and RS CVn-like variables are being observed with the Molonglo Observatory Synthesis Telescope in an attempt to detect quiescent (non-flaring) emission. Two flare stars out of 7 and one RS CVn out of 8 have been detected. Quiescent emission has not been observed previously from these sources at such a low frequency. All sources so far detected have mean flux densities below 10 mJy and in at least two of them the emission varies with a time scale of about one day.
    Original languageEnglish
    Pages (from-to)319-322
    Number of pages4
    JournalProceedings astronomical society of australia
    Issue number3
    Publication statusPublished - 1986


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