Mass loss from hot massive stars
J Puls, JS Vink, F Najarro - The Astronomy and Astrophysics Review, 2008 - Springer
Mass loss is a key process in the evolution of massive stars, and must be understood
quantitatively if it is to be successfully included in broader astrophysical applications such as …
quantitatively if it is to be successfully included in broader astrophysical applications such as …
Winds from hot stars
RP Kudritzki, J Puls - Annual Review of Astronomy and …, 2000 - annualreviews.org
▪ Abstract This review deals with the winds from “normal” hot stars such as O-stars, B-and A-
supergiants, and Central Stars of Planetary Nebulae with O-type spectra. The advanced …
supergiants, and Central Stars of Planetary Nebulae with O-type spectra. The advanced …
Time-dependent models of radiatively driven stellar winds. I-Nonlinear evolution of instabilities for a pure absorption model
SP Owocki, JI Castor, GB Rybicki - … ), vol. 335, Dec. 15, 1988, p …, 1988 - adsabs.harvard.edu
The authors describe results of numerical radiation-hydrodynamics simulations of the
nonlinear evolution of instabilities in radiatively driven stellar winds. The wind is idealized as …
nonlinear evolution of instabilities in radiatively driven stellar winds. The wind is idealized as …
Hydrodynamical simulations of corotating interaction regions and discrete absorption components in rotating O-star winds
SR Cranmer, SP Owocki - ar** factor in hot star winds from a combined H, IR and radio analysis
J Puls, N Markova, S Scuderi, C Stanghellini… - Astronomy & …, 2006 - aanda.org
Context. Recent results strongly challenge the canonical picture of massive star winds:
various evidence indicates that currently accepted mass-loss rates,, may need to be revised …
various evidence indicates that currently accepted mass-loss rates,, may need to be revised …
Dynamical simulations of magnetically channeled line-driven stellar winds. I. Isothermal, nonrotating, radially driven flow
SP Owocki - The Astrophysical Journal, 2002 - iopscience.iop.org
We present numerical magnetohydrodynamic (MHD) simulations of the effect of stellar
dipole magnetic fields on line-driven wind outflows from hot, luminous stars. Unlike previous …
dipole magnetic fields on line-driven wind outflows from hot, luminous stars. Unlike previous …
Towards a unified view of inhomogeneous stellar winds in isolated supergiant stars and supergiant high mass X-ray binaries
S Martínez-Núñez, P Kretschmar, E Bozzo… - Space Science …, 2017 - Springer
Massive stars, at least∼ 10 \sim10 times more massive than the Sun, have two key
properties that make them the main drivers of evolution of star clusters, galaxies, and the …
properties that make them the main drivers of evolution of star clusters, galaxies, and the …
[HTML][HTML] Advances in understanding high-mass X-ray binaries with INTEGRALand future directions
P Kretschmar, F Fürst, L Sidoli, E Bozzo… - New Astronomy …, 2019 - Elsevier
High mass X-ray binaries are among the brightest X-ray sources in the Milky Way, as well as
in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology …
in nearby Galaxies. Thanks to their highly variable emissions and complex phenomenology …
Time-dependent structure and energy transfer in hot star winds.
A Feldmeier - Astronomy and Astrophysics, v. 299, p. 523, 1995 - adsabs.harvard.edu
We present time-dependent hydrodynamical models of radiation driven hot star winds,
which are subject to a strong instability intrinsic to the radiative line force. The calculations …
which are subject to a strong instability intrinsic to the radiative line force. The calculations …
Long-and short-term variability in O-star winds. I. Time series of UV spectra for 10 bright O stars
L Kaper, HF Henrichs, JS Nichols, LC Snoek… - Astronomy and …, 1996 - aas.aanda.org
An atlas of time series of ultraviolet spectra is presented for 10 bright O stars. The spectra
were obtained with the International Ultraviolet Explorer during seven observing campaigns …
were obtained with the International Ultraviolet Explorer during seven observing campaigns …