We report on recent progress in our theoretical understanding of X-ray binaries, which has largely been driven by new observations, and illustrate the interplay between theory and observations considering as examples intermediate-mass X-ray binaries, irradiation-driven evolution, ultraluminous X-ray sources and neutron stars with low-velocity kicks
A short review of ultra-compact binaries, focused on ultra-compact X-ray binaries, is followed by a ...
Low-mass X-ray binaries dominate the energy X-ray output of our Galaxy. They are ideal systems to st...
One of the key open questions in high-energy astrophysics is understanding the complex relationship ...
X-ray astronomy is the prime available window on astrophysical compact objects: black holes, neutron...
This review summarizes the observational constraints on the mass spectrum of compact objects in X-ra...
A review of some properties of X-ray binaries is presented. The review is concentrated mainly on low...
Ultracompact X-ray binaries (UCXBs) appear able to sustain accretion onto the compact accretor at r...
In this thesis we investigate the formation and evolution of compact binaries. Chapters 2 through 4 ...
Abstract This thesis focuses on observational study of a variety of phenomena that occur in the vici...
International audienceX-ray observations of quiescent low-mass X-ray binaries (qLMXBs) provide one o...
Halfway the twentieth century, technological developments made it possible to carry detection instru...
n important advance in high-energy astrophysics over the past decade has been the detailed understan...
Compact and double compact binary systems are excellent natural laboratories for the study of a vari...
Context. Ultracompact X-ray binaries (UCXBs) typically consist of a white dwarf donor and a neutron ...
Short-period binaries run the gamut from widely separated stars to black-hole pairs; in between are ...
A short review of ultra-compact binaries, focused on ultra-compact X-ray binaries, is followed by a ...
Low-mass X-ray binaries dominate the energy X-ray output of our Galaxy. They are ideal systems to st...
One of the key open questions in high-energy astrophysics is understanding the complex relationship ...
X-ray astronomy is the prime available window on astrophysical compact objects: black holes, neutron...
This review summarizes the observational constraints on the mass spectrum of compact objects in X-ra...
A review of some properties of X-ray binaries is presented. The review is concentrated mainly on low...
Ultracompact X-ray binaries (UCXBs) appear able to sustain accretion onto the compact accretor at r...
In this thesis we investigate the formation and evolution of compact binaries. Chapters 2 through 4 ...
Abstract This thesis focuses on observational study of a variety of phenomena that occur in the vici...
International audienceX-ray observations of quiescent low-mass X-ray binaries (qLMXBs) provide one o...
Halfway the twentieth century, technological developments made it possible to carry detection instru...
n important advance in high-energy astrophysics over the past decade has been the detailed understan...
Compact and double compact binary systems are excellent natural laboratories for the study of a vari...
Context. Ultracompact X-ray binaries (UCXBs) typically consist of a white dwarf donor and a neutron ...
Short-period binaries run the gamut from widely separated stars to black-hole pairs; in between are ...
A short review of ultra-compact binaries, focused on ultra-compact X-ray binaries, is followed by a ...
Low-mass X-ray binaries dominate the energy X-ray output of our Galaxy. They are ideal systems to st...
One of the key open questions in high-energy astrophysics is understanding the complex relationship ...