A search for 843 MHz radio emission from active stars

Alan Vaughan; M. I. Large

A search for 843 MHz radio emission from active stars

Alan Vaughan, M. I. Large

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

Abstract

Known Southern flare stars and RS CVn-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 RS CVn 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.

Original language	English
Pages (from-to)	319-322
Number of pages	4
Journal	Proceedings astronomical society of australia
Volume	6
Issue number	3
Publication status	Published - 1986

Cite this

@article{71dca42d948e4195b0305a280438839e,

title = "A search for 843 MHz radio emission from active stars",

abstract = "Known Southern flare stars and RS CVn-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 RS CVn 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.",

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

year = "1986",

language = "English",

volume = "6",

pages = "319--322",

journal = "Proceedings astronomical society of australia",

issn = "0066-9997",

publisher = "C S I R O PUBLICATIONS",

number = "3",

}

TY - JOUR

T1 - A search for 843 MHz radio emission from active stars

AU - Vaughan, Alan

AU - Large, M. I.

PY - 1986

Y1 - 1986

N2 - Known Southern flare stars and RS CVn-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 RS CVn 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.

AB - Known Southern flare stars and RS CVn-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 RS CVn 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.

M3 - Article

SN - 0066-9997

VL - 6

SP - 319

EP - 322

JO - Proceedings astronomical society of australia

JF - Proceedings astronomical society of australia

IS - 3

ER -

A search for 843 MHz radio emission from active stars

Abstract

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