Do We Understand Wolf-Rayet Stars?

Details Do We Understand Wolf-Rayet Stars? Do We Understand Wolf-Rayet Stars?

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..171h&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

Astronomy and Astrophysics

Astronomy

Scientific paper

The spectra of Wolf-Rayet stars can be reproduced by line-blanketed model atmospheres. WR winds are strongly inhomogeneous; one means to study wind clumping is provided by the X-ray line profiles. First hydrodynamically consistent WR wind models now exist for some WR subtypes. The new evolutionary models for massive stars which account for rotation can still not reproduce well the Galactic WR population.

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