Far-UV wind line profile changes in the O-type star HD 175754

Details Far-UV wind line profile changes in the O-type star HD 175754 Far-UV wind line profile changes in the O-type star HD 175754

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26a...100..183c&link_type=abstract

Astronomy and Astrophysics, vol. 100, no. 1, July 1981, p. 183-185. Research supported by the Consiglio Nazionale delle Ricerch

Astronomy and Astrophysics

Astrophysics

1

Far Ultraviolet Radiation, O Stars, Stellar Spectra, Stellar Winds, Ultraviolet Spectra, Iue, Resonance Lines

Scientific paper

Resonance line profile changes in far-UV spectra of HD 175754, obtained
with the IUE satellite are reported. These changes are interpreted in
terms of variations in the dynamics and density-ionization structure of
the star's wind.

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