Among the different types of massive stars in advanced evolutionary stages is the enigmatic WN8h type. There are only a few Wolf–Rayet (WR) stars with this spectral type in our Galaxy. It has long been suggested that WN8h-type stars are the products of binary evolution that may harbor neutron stars (NS). One of the most intriguing WN8h stars is the runaway WR 124 surrounded by its magnificent nebula M1-67. We test the presence of an accreting NS companion in WR 124 using ~100 ks long observations by the Chandra X-ray observatory. The hard X-ray emission from WR 124 with a luminosity of L X ~ 1031 erg s−1 is marginally detected. We use the non-local thermodynamic equilibrium stellar atmosphere code PoWR to estimate the WR wind opacity to the...
WR 3 is the brightest very early-type WN star in the sky. Based on several years of time-resolved sp...
Aims. We study the distribution of Wolf-Rayet (WR) stars and their subtypes with respect to their ...
The explosive fate of massive Wolf-Rayet stars (WRSs) is a key open question in stellar physics. An ...
© 2018. The American Astronomical Society. All rights reserved.. Among the different types of massiv...
© 2018. The American Astronomical Society. All rights reserved.. Among the different types of massiv...
Among the different types of massive stars in advanced evolutionary stages is the enigmatic WN8h typ...
Context. Massive-binary evolution models predict that some systems will go through an evol...
Over a hundred planetary nebulae (PNe) are known to have H-deficient central stars that mimic the sp...
Context. Comprehensive studies of Wolf-Rayet stars were performed in the past for the Galactic and t...
Aims. To further investigate the nature of the enigmatic object WR 46 and better understan...
We report new results from our effort to identify obscured Wolf-Rayet stars in the Galaxy. Candidate...
Abstract We present an overview of recent X-ray obser-vations of Wolf-Rayet (WR) stars with XMM-Newt...
Aims: To further investigate the nature of the enigmatic object WR 46 and better understand the X-ra...
Context. Massive Wolf-Rayet (WR) stars are evolved massive stars (Mi ≳ 20 M⊙) characterized by stron...
Most population I Wolf-Rayet (WR) stars are the He-rich descendants of the most massive stars (M_i =...
WR 3 is the brightest very early-type WN star in the sky. Based on several years of time-resolved sp...
Aims. We study the distribution of Wolf-Rayet (WR) stars and their subtypes with respect to their ...
The explosive fate of massive Wolf-Rayet stars (WRSs) is a key open question in stellar physics. An ...
© 2018. The American Astronomical Society. All rights reserved.. Among the different types of massiv...
© 2018. The American Astronomical Society. All rights reserved.. Among the different types of massiv...
Among the different types of massive stars in advanced evolutionary stages is the enigmatic WN8h typ...
Context. Massive-binary evolution models predict that some systems will go through an evol...
Over a hundred planetary nebulae (PNe) are known to have H-deficient central stars that mimic the sp...
Context. Comprehensive studies of Wolf-Rayet stars were performed in the past for the Galactic and t...
Aims. To further investigate the nature of the enigmatic object WR 46 and better understan...
We report new results from our effort to identify obscured Wolf-Rayet stars in the Galaxy. Candidate...
Abstract We present an overview of recent X-ray obser-vations of Wolf-Rayet (WR) stars with XMM-Newt...
Aims: To further investigate the nature of the enigmatic object WR 46 and better understand the X-ra...
Context. Massive Wolf-Rayet (WR) stars are evolved massive stars (Mi ≳ 20 M⊙) characterized by stron...
Most population I Wolf-Rayet (WR) stars are the He-rich descendants of the most massive stars (M_i =...
WR 3 is the brightest very early-type WN star in the sky. Based on several years of time-resolved sp...
Aims. We study the distribution of Wolf-Rayet (WR) stars and their subtypes with respect to their ...
The explosive fate of massive Wolf-Rayet stars (WRSs) is a key open question in stellar physics. An ...