Abstract
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 language | English |
|---|---|
| Pages (from-to) | 319-322 |
| Number of pages | 4 |
| Journal | Proceedings astronomical society of australia |
| Volume | 6 |
| Issue number | 3 |
| Publication status | Published - 1986 |