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Wolf-Rayet stars

2008
Based on the so-called standard model for expanding atmospheres, non-LTE model calculations have been developed during the last years. Their application for the quantitative spectral analysis of WR stars is in progress. Recent results about the parameters and chemical composition of WR atmospheres are reviewed.
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The Wolf-Rayet stars and mass loss

Astrophysics and Space Science, 1969
Wolf-Rayet stars are defined, a summary is given of the properties of Wolf-Rayet stars, and a qualitative model of a Wolf-Rayet star is sketched. It is incontrovertible that Wolf-Rayet stars are losing mass, a typical rate of mass loss being near 10-5 M ⊙ per year.
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Analyses of Wolf-Rayet Stars

1990
Wolf-Rayet stars represent an important stage in the evolution of massive stars, but are only poorly understood so far. For a better knowledge one might determine their effective temperatures, luminosities and atmospheric compositions. But the emission-line dominated Wolf-Rayet spectra were not accessible to a quantitative analysis for a long time ...
W.-R. Hamann   +7 more
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The galactic distribution of Wolf-Rayet stars

ASTRONOMICAL JOURNAL OF AZERBAIJAN, 2023
Rustamov, J. N., Abdulkarimova, A. F.
openaire   +1 more source

Wolf—Rayet Stars

Astrophysics and Space Science, 1996
openaire   +2 more sources

On the bipolarity of Wolf–Rayet nebulae

Monthly Notices of the Royal Astronomical Society, 2021
Dominique M -A Meyer
exaly  

On the nature of massive helium star winds and Wolf–Rayet-type mass-loss

Monthly Notices of the Royal Astronomical Society, 2020
Andreas Sander, Jorick Sándor Vink
exaly  

The Wolf-Rayet Stars

Publications of the Astronomical Society of the Pacific, 1929
openaire   +1 more source

First 3D radiation-hydrodynamic simulations of Wolf-Rayet winds

Astronomy and Astrophysics, 2022
Nathaniel Kee   +2 more
exaly  

Physical Properties of Wolf-Rayet Stars

Annual Review of Astronomy and Astrophysics, 2007
Paul Crowther
exaly  

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