843 MHZ 843 MHZ emission from the active star-AB-DOR

A. J. Beasley, M. I. Large, Alan Vaughan

Research output: Contribution to journalArticle

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 languageEnglish
Pages (from-to)46-49
Number of pages4
JournalProceedings astronomical society of australia
Volume7
Issue number1
Publication statusPublished - 1987

Cite this

Beasley, A. J., Large, M. I., & Vaughan, A. (1987). 843 MHZ 843 MHZ emission from the active star-AB-DOR. Proceedings astronomical society of australia, 7(1), 46-49.