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...
Are WO-type Wolf Rayet (WR) stars in the final stage of massive star evolution before core-collapse?...
The explosive fate of massive Wolf-Rayet stars (WRSs) is a key open question in stellar physics. An ...
With a deep Chandra/HETGS exposure of WR 6, we have resolved emission lines whose profiles show that...
Among the different types of massive stars in advanced evolutionary stages is the enigmatic WN8h typ...
© 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...
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...
The carbon-rich WC5 star WR 114 was not detected during a 15.9 ksec XMM-Newton observation, implying...
We present the results of an XMM-Newton observation of the field of the Wolf-Rayet star WR 40. Despi...
Context. The classical Wolf-Rayet (WR) phase is believed to mark the end stage of the evolution of m...
We report the discovery of weak yet hard X-ray emission from the Wolf-Rayet (WR) star WR 142 with th...
We present results of an ≈20-ks X-ray observation of the Wolf-Rayet (WR) binary system WR 147 obtain...
Context. Massive Wolf-Rayet (WR) stars are evolved massive stars (Mi ≳ 20 M⊙) characterized by stron...
We have spectroscopically discovered a pair of twin, nitrogen-type, hydrogen-rich, Wolf-Rayet stars ...
Are WO-type Wolf Rayet (WR) stars in the final stage of massive star evolution before core-collapse?...
The explosive fate of massive Wolf-Rayet stars (WRSs) is a key open question in stellar physics. An ...
With a deep Chandra/HETGS exposure of WR 6, we have resolved emission lines whose profiles show that...
Among the different types of massive stars in advanced evolutionary stages is the enigmatic WN8h typ...
© 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...
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...
The carbon-rich WC5 star WR 114 was not detected during a 15.9 ksec XMM-Newton observation, implying...
We present the results of an XMM-Newton observation of the field of the Wolf-Rayet star WR 40. Despi...
Context. The classical Wolf-Rayet (WR) phase is believed to mark the end stage of the evolution of m...
We report the discovery of weak yet hard X-ray emission from the Wolf-Rayet (WR) star WR 142 with th...
We present results of an ≈20-ks X-ray observation of the Wolf-Rayet (WR) binary system WR 147 obtain...
Context. Massive Wolf-Rayet (WR) stars are evolved massive stars (Mi ≳ 20 M⊙) characterized by stron...
We have spectroscopically discovered a pair of twin, nitrogen-type, hydrogen-rich, Wolf-Rayet stars ...
Are WO-type Wolf Rayet (WR) stars in the final stage of massive star evolution before core-collapse?...
The explosive fate of massive Wolf-Rayet stars (WRSs) is a key open question in stellar physics. An ...
With a deep Chandra/HETGS exposure of WR 6, we have resolved emission lines whose profiles show that...