The winds and coronae of early-type stars

Details The winds and coronae of early-type stars The winds and coronae of early-type stars

Nov 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nascp.2280.263c&link_type=abstract

In JPL Solar Wind Five p 263-278 (SEE N84-13067 03-92)

Astronomy and Astrophysics

Astronomy

1

Early Stars, Emission Spectra, Line Spectra, Stellar Coronas, Stellar Winds, Radio Astronomy, Stellar Temperature, Ultraviolet Astronomy, Wind Profiles, X Ray Astronomy

Scientific paper

The properties of the winds of hot stars as derived from radio, ultraviolet and X-ray observations are presented. Special focus is given to observations that test line driven wind theory. In this theory the wind properties are determined by the stellar effective temperature and surface gravity, but not parameters that specify the mechanical or wave fluxes from the star. Alternate explanations of the X-ray emission from the early-type stars are discussed. Evidence is given for the presence of coronal zones at the base of the stellar winds.

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