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Observations of Active Stars at 843 MHz

Published online by Cambridge University Press:  25 April 2016

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

The Molonglo Observatory Synthesis Telescope is being used in a continuing program of observation of known Southern active stars. By May, 1987, a total of forty-one stars had been observed and 843 MHz quiescent emission, presumably associated with the star, had been detected in nine instances. The emission from five of these stars has shown marked variation on a time-scale > 1 day.

Type
Stellar
Information
Publications of the Astronomical Society of Australia , Volume 7 , Issue 1 , 1987 , pp. 42 - 45
Copyright
Copyright © Astronomical Society of Australia 1987

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References

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