Abstract
The Molonglo Observatory synthesis telescope has been used to obtain twelve observations of a 23arcmin arc field containing the active star AB Dor. On each occasion, an unresolved source close to the optical position of AB Dor was observed. The source exhibits day-to-day variations of flux density, with a mean value of ≡4 mJy. The identification of the source with the star and the variations in emission are discussed.
| Original language | English |
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| Pages (from-to) | 46-49 |
| Number of pages | 4 |
| Journal | Proceedings astronomical society of australia |
| Volume | 7 |
| Issue number | 1 |
| Publication status | Published - 1987 |