Ultraviolet spectral morphology of O-type stellar winds

Details Ultraviolet spectral morphology of O-type stellar winds Ultraviolet spectral morphology of O-type stellar winds

Jan 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985nascp2358...66w&link_type=abstract

In NASA. Goddard Space Flight Center The Origin of Nonradiative Heating/Momentum in Hot Stars p 66-69 (SEE N85-17755 08-88)

Astronomy and Astrophysics

Astronomy

Stars, Stellar Models, Stellar Winds, Ultraviolet Spectra, Iue, Line Spectra, Stellar Luminosity, Ultraviolet Astronomy

Scientific paper

The highly systematic behavior of the stellar wind features among the majority of O-type spectra, and their strong correlations with the well-calibrated optical spectral types, are consistent with those wind models which incorporate a structural dependence on the fundamental stellar parameters. On the contrary, wind models which postulate a predominance of random rotational or magnetic effects, unrelated to the fundamental stellar parameters, are not supported by the ultraviolet spectral morphology; rather, such effects may contribute to the observed properties of some of the exceptionally peculiar objects.

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