Radio Observations of Early-Type Stars

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Scientific paper

A survey of 32 O, B, and Wolf-Rayet stars with the NRAO interferometer failed to detect unresolved radio sources coincident with any of the stellar positions. The detection limits range from 10 to 50 x 10-29 W m-2 Hz-1. Consequently, the physical processes that produce the radio radiation observed in other types of stars are not as important for early-type stars. Limits on physical conditions near the star are derived. The nature of the 'superbright radio knots' observed by Miley et al.,is briefly discussed.

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