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A Very Large Array 3.6 Centimeter Continuum Survey of Galactic Wolf-Rayet Stars
2004
Astronomical Journal
We report the results of a survey of radio continuum emission of Galactic Wolf-Rayet stars north of declination -46 degrees. The observations were obtained at 8.46 GHz (3.6cm) using the Very Large Array (VLA), with an angular resolution of about 6 x 9 arcsec and typical rms noise of 0.04 mJy/beam. Our survey of 34 WR stars resulted in 15 definite and 5 probable detections, 13 of these for the first time at radio wavelengths. All detections are unresolved. Time variations in flux are confirmed
doi:10.1086/383286
fatcat:yzvgovmdyjajrcf425webg4rku