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

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

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

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

Research output: Contribution to journal › Article › peer-review

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
Pages (from-to)	46-49
Number of pages	4
Journal	Proceedings astronomical society of australia
Volume	7
Issue number	1
Publication status	Published - 1987

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@article{6e4ab487e8624de8b19d2e06812ea7dc,

title = "843 MHZ 843 MHZ emission from the active star-AB-DOR",

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.",

author = "Beasley, \{A. J.\} and Large, \{M. I.\} and Alan Vaughan",

year = "1987",

language = "English",

volume = "7",

pages = "46--49",

journal = "Proceedings astronomical society of australia",

issn = "0066-9997",

publisher = "C S I R O PUBLICATIONS",

number = "1",

}

TY - JOUR

T1 - 843 MHZ 843 MHZ emission from the active star-AB-DOR

AU - Beasley, A. J.

AU - Large, M. I.

AU - Vaughan, Alan

PY - 1987

Y1 - 1987

N2 - 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.

AB - 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.

M3 - Article

SN - 0066-9997

VL - 7

SP - 46

EP - 49

JO - Proceedings astronomical society of australia

JF - Proceedings astronomical society of australia

IS - 1

ER -

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

Abstract

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