Keywords
Early-Type Stars:Line Profiles
Early-Type Stars:Stellar Winds
Early-Type Stars:UV Spectra
Line Profiles:Early-Type Stars
Stellar Winds:Early-Type Stars
UV Spectra:Early-Type Stars
Early-Type Stars:Stellar Winds
Early-Type Stars:UV Spectra
Line Profiles:Early-Type Stars
Stellar Winds:Early-Type Stars
UV Spectra:Early-Type Stars
How to Cite
Resonance line-profiles in galactic disk UV-bright stars. (1987). Revista Mexicana De Astronomía Y Astrofísica, 14(1), 301-309. https://astronomia.unam.mx/journals/rmxaa/article/view/1987rmxaa..14..301c
Abstract
The authors have made a comparative analysis of UV resonance line-profiles in O-type stars members of young clusters and OB associations, with those of hot stars located away from sites of recent star formation (including "runaway" stars). The resonance line-profiles are found to be generally dominated by stellar winds that appear to depend mainly on the surface gravity and temperature of the star, and not on its mass. The use of only the largest stellar wind velocity detectable in the resonance lines as a stellar population indicator, is disputed.Similar Articles
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