Observations of nonthermal radio emission from early-type stars

Details Observations of nonthermal radio emission from early-type stars Observations of nonthermal radio emission from early-type stars

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358...47a&link_type=abstract

In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 47-52 (SEE N85-17755 08-88)

Statistics

Early Stars, Emission Spectra, Nonthermal Radiation, Radio Emission, Stellar Winds, Wolf-Rayet Stars, Estimates, Stellar Luminosity, Thermal Emission

Scientific paper

As a part of a wider survey of radio emission from O, B, and Wolf-Rayet (WR) stars, five new stars whose radio emission is dominated by a nonthermal mechanism of unknown origin were discovered. From statistics of distance-limited samples of stars, it is estimated that the minimum fraction of stars which are nonthermal emitters is 25% for the OB stars and 10% for the WR stars. The characteristics of this new class of nonthermal radio emitter are investigated.

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