Runacres, M. ; Blomme, R.

published in Astrophysics and Space Science, 221, pp. 249-257 (1994)

Abstract: 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.

DOI: 10.1007/BF01091157
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