Abstract
The Molonglo Observatory Synthesis Telescope is being used in a continuing program of observation of known southern active stars. By May, 1987, a total of forty-one stars had been observed and 843 MHz quiescent emission, presumably associated with the star, had been detected in nine instances. The emission from five of these stars has shown marked variation on a time-scale >1 day.
| Original language | English |
|---|---|
| Pages (from-to) | 42-45 |
| Number of pages | 4 |
| Journal | Proceedings astronomical society of australia |
| Volume | 7 |
| Issue number | 1 |
| Publication status | Published - 1987 |