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 ζ Pup appears to show an effect of clumping in its continuum flux.
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© 1994 Springer Science+Business Media Dordrecht
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Runacres, M., Blomme, R. (1994). The Infrared and Radio Continuum of OB-Stars. In: Moffat, A.F.J., Owocki, S.P., Fullerton, A.W., St-Louis, N. (eds) Instability and Variability of Hot-Star Winds. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-0315-2_19
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DOI: https://doi.org/10.1007/978-94-011-0315-2_19
Publisher Name: Springer, Dordrecht
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