The Winds of O-Type Stars: Ionization Structure and Revised Stellar Parameters from Far-UV Spectra

Details The Winds of O-Type Stars: Ionization Structure and Revised Stellar Parameters from Far-UV Spectra The Winds of O-Type Stars: Ionization Structure and Revised Stellar Parameters from Far-UV Spectra

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..226b&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

3

Stars: Early-Type, Stars: Fundamental Parameters, Stars: Mass Loss, Stars: Winds, Outflows

Scientific paper

We derived consistent photospheric and wind parameters of O-type stars,
by analyzing high-resolution spectra in the range 905 to 3250 Å
with line-blanketed, hydrodynamic, non-LTE spherical models. We find
significantly lower T[eff] and luminosities than previously assigned to
these spectral types.

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