Add to ORKGWe study the influence of X-ray radiation on the wind parameters of O stars. For this purpose we use our own NLTE wind code. The X-ray emission (assumed to be generated in wind shocks) is treated as an input quantity. We study its influence on the mass-loss rate, terminal velocity and ionization state of the stellar wind of Galactic O stars
The principal aim of this project was to determine whether x ray emission from instability-generated...
OB stars with strong radiation-driven stellar winds and large-scale magnetic fields generate strong ...
Context. Extreme ultraviolet (EUV) and X-ray radiation emitted from wind-embedded shocks in hot, mas...
X-rays give direct evidence of instabilities, time-variable structure, and shock heating in the wind...
Context. Binaries with hot massive components are strong X-ray sources. Besides the intrinsic X-ray ...
peer reviewedHigh-resolution X-ray spectra of O-type stars revealed less wind absorption than expect...
Young O stars are strong, hard, and variable X-ray sources, properties which strongly a®ect their ci...
Young O stars are strong, hard, and variable X-ray sources, properties which strongly affect their c...
High-resolution X-ray grating spectroscopy enables us to measure the kinematics and spatial distribu...
A semi-empirical model is developed for the X-ray emission from O star winds, and used to analyze re...
[[abstract]]In order to compare the X-wind with observations, one needs to be able to calculate its ...
O stars are highly important objects in their host galaxies due to the impact of their powerful ste...
Copyright © 2000 Royal Astronomical SocietyWe review existing ROSAT detections of single Galactic Wo...
XMM-Newton observations of the O supergiant zeta Orionis (O9.7 Ib) extend knowledge of its high-reso...
In order to compare the x-wind with observations, one needs to be able to calculate its thermal and ...
The principal aim of this project was to determine whether x ray emission from instability-generated...
OB stars with strong radiation-driven stellar winds and large-scale magnetic fields generate strong ...
Context. Extreme ultraviolet (EUV) and X-ray radiation emitted from wind-embedded shocks in hot, mas...
X-rays give direct evidence of instabilities, time-variable structure, and shock heating in the wind...
Context. Binaries with hot massive components are strong X-ray sources. Besides the intrinsic X-ray ...
peer reviewedHigh-resolution X-ray spectra of O-type stars revealed less wind absorption than expect...
Young O stars are strong, hard, and variable X-ray sources, properties which strongly a®ect their ci...
Young O stars are strong, hard, and variable X-ray sources, properties which strongly affect their c...
High-resolution X-ray grating spectroscopy enables us to measure the kinematics and spatial distribu...
A semi-empirical model is developed for the X-ray emission from O star winds, and used to analyze re...
[[abstract]]In order to compare the X-wind with observations, one needs to be able to calculate its ...
O stars are highly important objects in their host galaxies due to the impact of their powerful ste...
Copyright © 2000 Royal Astronomical SocietyWe review existing ROSAT detections of single Galactic Wo...
XMM-Newton observations of the O supergiant zeta Orionis (O9.7 Ib) extend knowledge of its high-reso...
In order to compare the x-wind with observations, one needs to be able to calculate its thermal and ...
The principal aim of this project was to determine whether x ray emission from instability-generated...
OB stars with strong radiation-driven stellar winds and large-scale magnetic fields generate strong ...
Context. Extreme ultraviolet (EUV) and X-ray radiation emitted from wind-embedded shocks in hot, mas...