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843 MHz Emission from the Active Star AB Dor
Published online by Cambridge University Press: 25 April 2016
Abstract
The Molonglo Observatory synthesis telescope has been used to obtain twelve observations of a 23′ 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.
- Type
- Stellar
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- Copyright © Astronomical Society of Australia 1987
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