International audienceIn the last decade, X-ray spectroscopy has enabled a wealth of discoveries of photoionised absorbers in X-ray binaries. Studies of such accretion disc atmospheres and winds are of fundamental importance to understand accretion processes and possible feedback mechanisms to the environment. In this work, we review the current observational state and theoretical understanding of accretion disc atmospheres and winds in low-mass X-ray binaries, focusing on the wind launching mechanisms and on the dependence on accretion state. We conclude with issues that deserve particular attention. (© 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim
Accretion in white-dwarf binary systems can occur through discs, accretion columns or a combination ...
Three classical modes of accretion are briefly discussed: wind-fed, spherical, and disk. The three m...
We consider modulations of mass captured by the compact object from the companion star’s stellar win...
International audienceIn the last decade, X-ray spectroscopy has enabled a wealth of discoveries of ...
We review the current status of studies of disc atmospheres and winds in low mass X-ray binaries. We...
We have carried out radiation-hydrodynamic simulations of thermally-driven accretion disc winds in l...
We have carried out radiation-hydrodynamic simulations of thermally driven accretion disc winds in l...
Low-mass X-ray binaries (LMXB) are stellar systems where a compact object accretes mass from a low-m...
Accretion onto compact objects of material from strong stellar winds, be it in High-Mass X-ray Binar...
The transport processes governing the phenomenology of accretion discs remain elusive as ever, even ...
The advent of the new generation of X-ray telescopes yielded a significant step forward in our under...
MAXI J1348-630 is a low mass X-ray binary discovered in 2019 during a bright outburst. During this e...
MAXI J1348–630 is a low mass X-ray binary discovered in 2019 during a bright outburst. During this e...
We present the results of a theoretical study investigating the effects of photoionization and heati...
In this thesis I present the results of my PhD research into the physics of accretion (infall) and e...
Accretion in white-dwarf binary systems can occur through discs, accretion columns or a combination ...
Three classical modes of accretion are briefly discussed: wind-fed, spherical, and disk. The three m...
We consider modulations of mass captured by the compact object from the companion star’s stellar win...
International audienceIn the last decade, X-ray spectroscopy has enabled a wealth of discoveries of ...
We review the current status of studies of disc atmospheres and winds in low mass X-ray binaries. We...
We have carried out radiation-hydrodynamic simulations of thermally-driven accretion disc winds in l...
We have carried out radiation-hydrodynamic simulations of thermally driven accretion disc winds in l...
Low-mass X-ray binaries (LMXB) are stellar systems where a compact object accretes mass from a low-m...
Accretion onto compact objects of material from strong stellar winds, be it in High-Mass X-ray Binar...
The transport processes governing the phenomenology of accretion discs remain elusive as ever, even ...
The advent of the new generation of X-ray telescopes yielded a significant step forward in our under...
MAXI J1348-630 is a low mass X-ray binary discovered in 2019 during a bright outburst. During this e...
MAXI J1348–630 is a low mass X-ray binary discovered in 2019 during a bright outburst. During this e...
We present the results of a theoretical study investigating the effects of photoionization and heati...
In this thesis I present the results of my PhD research into the physics of accretion (infall) and e...
Accretion in white-dwarf binary systems can occur through discs, accretion columns or a combination ...
Three classical modes of accretion are briefly discussed: wind-fed, spherical, and disk. The three m...
We consider modulations of mass captured by the compact object from the companion star’s stellar win...