Upper limits to the radio-fluxes of the Wolf-Rayet stars WR 46 (WN3p) and WR 50 (WC7+abs)
Received 1 September 2000 / Accepted 22 September 2000
We have observed the Wolf-Rayet stars WR 46 (WN3p+c) and WR 50 (WC7+abs) at 3 and 6 cm using the Australia Telescope in search of non-thermal radio emission. However, the sources were not detected and we derive upper limits to their radio fluxes of 0.18 mJy (0.15 mJy in the case of WR 46 at 6 cm). These are not in conflict with expected thermal emission, because the wind densities have been found to be lower than an average WR wind. Inversely, assuming the mass-loss rate as determined from optical spectral analyses, the inferred lower limits to the distances are in agreement with previous determinations. Both objects are reported as short-period photometric variables, but we note that the variability of WR 50 is suspicious.
Key words: stars: Wolf-Rayet stars: individual: WR 46 = HD104994 stars: individual: WR 50 radio continuum: stars
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© European Southern Observatory (ESO) 2000
Online publication: December 5, 2000