The properties of stars showing Wolf-Rayet phenomena are outlined along with the direction of future work. Emphasis is placed on the characteristics of W-R spectra. Specifically the following topics are covered: the absolute visual magnitudes; the heterogeneity of WN spectra; the existence of transition type spectra and compositions the mass loss rates; and the existence of very luminous and possibly very massive W-R stars. Also, a brief overview of current understanding of the theoretical aspects of stellar evolution and stellar winds and the various scenarios that have been proposed to understand W-R spectra are included
Wolf-Rayet (WR) stars, as they are advanced stages of the life of massive stars, provide a good test...
Context. Most massive stars reside in multiple systems that will interact over the course of their l...
Context. Wolf-Rayet (WR) stars have a severe impact on their environments owing to their strong ioni...
The striking broad emission line spectroscopic appearance of Wolf-Rayet stars have long defied analy...
New high-resolution 1.0 - 3.4 pm spectra of carbon-rich Wolf-Rayet stars (W C ) are presen...
Recent results for Galactic and Magellanic Cloud Wolf-Rayet stars are summarised based on line blank...
Recent results with the Potsdam Wolf-Rayet (PoWR) models have shown that Wolf-Rayet mass loss can be...
We’ve recently completed searches for Wolf-Rayet (WR) stars in the Local Group galaxies including M3...
New observational data are given for the spectra of several Wolf-Rayet stars. Evidence is produced f...
Wolf-Rayet (WR) stars comprise a class of stars whose spectra are dominated by strong, broad emissio...
Context. Most massive stars reside in multiple systems that will interact over the course of their l...
Context. Most massive stars reside in multiple systems that will interact over the course of their l...
Context. Massive stars, although being important building blocks of galaxies, are still not fully un...
Observed properties of Wolf-Rayet stars at high metallicity are reviewed. Wolf-Rayet stars are more ...
Context.Very massive stars pass through the Wolf-Rayet (WR) stage before they finally explode. Detai...
Wolf-Rayet (WR) stars, as they are advanced stages of the life of massive stars, provide a good test...
Context. Most massive stars reside in multiple systems that will interact over the course of their l...
Context. Wolf-Rayet (WR) stars have a severe impact on their environments owing to their strong ioni...
The striking broad emission line spectroscopic appearance of Wolf-Rayet stars have long defied analy...
New high-resolution 1.0 - 3.4 pm spectra of carbon-rich Wolf-Rayet stars (W C ) are presen...
Recent results for Galactic and Magellanic Cloud Wolf-Rayet stars are summarised based on line blank...
Recent results with the Potsdam Wolf-Rayet (PoWR) models have shown that Wolf-Rayet mass loss can be...
We’ve recently completed searches for Wolf-Rayet (WR) stars in the Local Group galaxies including M3...
New observational data are given for the spectra of several Wolf-Rayet stars. Evidence is produced f...
Wolf-Rayet (WR) stars comprise a class of stars whose spectra are dominated by strong, broad emissio...
Context. Most massive stars reside in multiple systems that will interact over the course of their l...
Context. Most massive stars reside in multiple systems that will interact over the course of their l...
Context. Massive stars, although being important building blocks of galaxies, are still not fully un...
Observed properties of Wolf-Rayet stars at high metallicity are reviewed. Wolf-Rayet stars are more ...
Context.Very massive stars pass through the Wolf-Rayet (WR) stage before they finally explode. Detai...
Wolf-Rayet (WR) stars, as they are advanced stages of the life of massive stars, provide a good test...
Context. Most massive stars reside in multiple systems that will interact over the course of their l...
Context. Wolf-Rayet (WR) stars have a severe impact on their environments owing to their strong ioni...