Observations at 843 MHZ of quiescent emission from the flare star AT Mic

Alan Vaughan; M. I. Large

Observations at 843 MHZ of quiescent emission from the flare star AT Mic

Alan Vaughan, M. I. Large

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Abstract

The Molonglo Observatory Synthesis Telescope was used in 1983 and on four occasions in 1985 to map the 843-MHz continuum emission from a field including the flare star AT Mic. Quiescent emission, apparently from the star, was detected. The flux density varied from one observation to another, in the range 3 to 8 mJy at 843 MHz. These observations are thought to be the first reported of quiescent emission from a flare star at such a low frequency. The emission mechanism is not known.

Original language	English
Pages (from-to)	399-403
Number of pages	5
Journal	Monthly Notices of the Royal Astronomical Society
Volume	223
Issue number	2
Publication status	Published - 15 Nov 1986

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@article{26dd08e86fa9436cbc11971e0f8d2359,

title = "Observations at 843 MHZ of quiescent emission from the flare star AT Mic",

abstract = "The Molonglo Observatory Synthesis Telescope was used in 1983 and on four occasions in 1985 to map the 843-MHz continuum emission from a field including the flare star AT Mic. Quiescent emission, apparently from the star, was detected. The flux density varied from one observation to another, in the range 3 to 8 mJy at 843 MHz. These observations are thought to be the first reported of quiescent emission from a flare star at such a low frequency. The emission mechanism is not known.",

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

year = "1986",

month = nov,

day = "15",

language = "English",

volume = "223",

pages = "399--403",

journal = "Monthly Notices of the Royal Astronomical Society",

issn = "0035-8711",

publisher = "Oxford University Press",

number = "2",

}

TY - JOUR

T1 - Observations at 843 MHZ of quiescent emission from the flare star AT Mic

AU - Vaughan, Alan

AU - Large, M. I.

PY - 1986/11/15

Y1 - 1986/11/15

N2 - The Molonglo Observatory Synthesis Telescope was used in 1983 and on four occasions in 1985 to map the 843-MHz continuum emission from a field including the flare star AT Mic. Quiescent emission, apparently from the star, was detected. The flux density varied from one observation to another, in the range 3 to 8 mJy at 843 MHz. These observations are thought to be the first reported of quiescent emission from a flare star at such a low frequency. The emission mechanism is not known.

AB - The Molonglo Observatory Synthesis Telescope was used in 1983 and on four occasions in 1985 to map the 843-MHz continuum emission from a field including the flare star AT Mic. Quiescent emission, apparently from the star, was detected. The flux density varied from one observation to another, in the range 3 to 8 mJy at 843 MHz. These observations are thought to be the first reported of quiescent emission from a flare star at such a low frequency. The emission mechanism is not known.

M3 - Article

SN - 0035-8711

VL - 223

SP - 399

EP - 403

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 2

ER -

Observations at 843 MHZ of quiescent emission from the flare star AT Mic

Abstract

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