Results 101 to 110 of about 180 (127)
Some of the next articles are maybe not open access.
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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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, 1969Wolf-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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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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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, 2023Rustamov, J. N., Abdulkarimova, A. F.
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On the bipolarity of Wolf–Rayet nebulae
Monthly Notices of the Royal Astronomical Society, 2021Dominique M -A Meyer
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On the nature of massive helium star winds and Wolf–Rayet-type mass-loss
Monthly Notices of the Royal Astronomical Society, 2020Andreas Sander, Jorick Sándor Vink
exaly
First 3D radiation-hydrodynamic simulations of Wolf-Rayet winds
Astronomy and Astrophysics, 2022Nathaniel Kee +2 more
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Physical Properties of Wolf-Rayet Stars
Annual Review of Astronomy and Astrophysics, 2007Paul Crowther
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