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A Search for 843 MHz Radio Emission from Active Stars

Published online by Cambridge University Press:  25 April 2016

A. E. Vaughan  and
M. I. Large
A. E. Vaughan
Affiliation:
School of Mathematics and Physics, Macquarie University
M. I. Large
Affiliation:
School of Physics, University of Sydney
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Abstract

Known Southern flare stars and RSCVn-like variables are being observed with the Molonglo Observatory Synthesis Telescope in an attempt to detect quiescent (non-flaring) emission. Two flare stars out of 7 and one RSCVn out of 8 have been detected. Quiescent emission has not been observed previously from these sources at such a low frequency. All sources so far detected have mean flux densities below 10 mJy and in at least two of them the emission varies with a time scale of about one day.

Information

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 3 , 1986 , pp. 319 - 322
Copyright
Copyright © Astronomical Society of Australia 1986

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References

McLean, D. J. and Labrum, N. R., eds., ‘Solar Radiophysics —Studies of Emission from the Sun at Metre Wavelengths’. Cambridge University Press (1985).Google Scholar
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Slee, O. B., 1985, Private communication.Google Scholar
Vaughan, A. E. and Large, M. I., 1986, In preparation.Google Scholar