The infrared and radio continuum of OB-stars

Details The infrared and radio continuum of OB-stars The infrared and radio continuum of OB-stars

Nov 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.221..249r&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 221, no. 1-2, p. 249-257

Astronomy and Astrophysics

Astronomy

3

B Stars, Infrared Astronomy, O Stars, Radio Astronomy, Stellar Mass, Stellar Physics, Stellar Spectra, Stellar Structure, Stellar Winds, Infrared Astronomy Satellite, Infrared Spectra, Mass Distribution, Radio Emission, Spaceborne Astronomy, Stellar Models

Scientific paper

The infrared and radio continuum fluxes of a number of OB-stars are
compared to theoretical models. This gives us information about the mass
loss rates and the structure of the stellar wind. The more extreme
O-star zeta Pup appears to show an effect of clumping in its continuum
flux.

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