Add to ORKGInternational audienceIn this contribution we give a brief overview of the effects of rotation, stellar winds, metallicity and binarity on the evolution of massive stars. We focus on the role of these parameters in shaping the end states of stellar evolution. Special attention is given to the mass of the stellar remnants that has been questionned by the detection of heavy black holes in merger events leading to gravitational waves emission
The evolutionary models of massive stars that are widely used in various branches of astronomy are s...
Gravitational waves (GW) emitted by merging black holes (BH) and neutron stars are now routinely det...
Galactic nuclei are often found to contain young stellar populations and, in most cases, a central s...
International audienceIn this contribution we give a brief overview of the effects of rotation, stel...
International audienceIn this contribution we give a brief overview of the effects of rotation, stel...
International audienceIn this contribution we give a brief overview of the effects of rotation, stel...
Massive stars play a critical role in the evolution of galaxies and star clusters. Recent observatio...
Context. The first directly detected gravitational waves (GW 150914) were emitted by two coalescing ...
We construct evolutionary tracks for massive black hole binaries (MBHBs) embedded in a surrounding d...
We construct evolutionary tracks for massive black hole binaries (MBHBs) embedded in a surrounding d...
Abstract: Before binary components interact, they evolve as single stars do. We therefore first crit...
We calculate new evolutionary models of rotating primordial very massive stars, with initial mass fr...
Making the most of the rapidly increasing population of gravitational-wave detections of black hole ...
We construct evolutionary tracks for massive black hole binaries (MBHBs) embedded in a surround-ing ...
We study the orbital evolution and gravitational wave (GW) emission of supermassive black hole (SMBH...
The evolutionary models of massive stars that are widely used in various branches of astronomy are s...
Gravitational waves (GW) emitted by merging black holes (BH) and neutron stars are now routinely det...
Galactic nuclei are often found to contain young stellar populations and, in most cases, a central s...
International audienceIn this contribution we give a brief overview of the effects of rotation, stel...
International audienceIn this contribution we give a brief overview of the effects of rotation, stel...
International audienceIn this contribution we give a brief overview of the effects of rotation, stel...
Massive stars play a critical role in the evolution of galaxies and star clusters. Recent observatio...
Context. The first directly detected gravitational waves (GW 150914) were emitted by two coalescing ...
We construct evolutionary tracks for massive black hole binaries (MBHBs) embedded in a surrounding d...
We construct evolutionary tracks for massive black hole binaries (MBHBs) embedded in a surrounding d...
Abstract: Before binary components interact, they evolve as single stars do. We therefore first crit...
We calculate new evolutionary models of rotating primordial very massive stars, with initial mass fr...
Making the most of the rapidly increasing population of gravitational-wave detections of black hole ...
We construct evolutionary tracks for massive black hole binaries (MBHBs) embedded in a surround-ing ...
We study the orbital evolution and gravitational wave (GW) emission of supermassive black hole (SMBH...
The evolutionary models of massive stars that are widely used in various branches of astronomy are s...
Gravitational waves (GW) emitted by merging black holes (BH) and neutron stars are now routinely det...
Galactic nuclei are often found to contain young stellar populations and, in most cases, a central s...