MESA inlists associated with Berardo et al. (2017). MESA version 7624. Publication DOI: 10.3847/1538-4357/834/2/14
We have analysed two cosmological zoom simulations with $M_{\rm vir}\sim 10^{12}{\rm\,M}_\odot$ from...
We use hydrodynamical simulations of galaxy clusters and groups to study the effect of pre-heating o...
The luminosity of young giant planets can inform about their formation and accretion history. The di...
We calculate the evolution of gas giant planets during the runaway gas accretion phase of formation,...
The formation of galaxy clusters is not a unique process. Due to the assembling by mergers and accre...
International audienceContext. Galaxy clusters are the most recent products of hierarchical accretio...
The entropy distribution of the intracluster medium and the shape of its confining potential well co...
Abstract This paper is devoted to discuss the difference in the thermodynamic entropy budget per bar...
The formation history of giant planets determines their primordial structure and consequent evolutio...
23 pages, 18 figures, Accepted for publication in A&AInternational audienceStar formation in galaxie...
The generalized second law of thermodynamics states that entropy always increases when all event hor...
Context. Galaxy clusters are the most recent products of hierarchical accretion over cosmological sc...
Numerical simulations show that the migration of growing planetary cores may be dominated by turbule...
Gas processes affecting star formation are reviewed with an emphasis on gravitational and magnetic i...
In this work, we investigate the dynamical evolution of spherical self-gravitating systems under the...
We have analysed two cosmological zoom simulations with $M_{\rm vir}\sim 10^{12}{\rm\,M}_\odot$ from...
We use hydrodynamical simulations of galaxy clusters and groups to study the effect of pre-heating o...
The luminosity of young giant planets can inform about their formation and accretion history. The di...
We calculate the evolution of gas giant planets during the runaway gas accretion phase of formation,...
The formation of galaxy clusters is not a unique process. Due to the assembling by mergers and accre...
International audienceContext. Galaxy clusters are the most recent products of hierarchical accretio...
The entropy distribution of the intracluster medium and the shape of its confining potential well co...
Abstract This paper is devoted to discuss the difference in the thermodynamic entropy budget per bar...
The formation history of giant planets determines their primordial structure and consequent evolutio...
23 pages, 18 figures, Accepted for publication in A&AInternational audienceStar formation in galaxie...
The generalized second law of thermodynamics states that entropy always increases when all event hor...
Context. Galaxy clusters are the most recent products of hierarchical accretion over cosmological sc...
Numerical simulations show that the migration of growing planetary cores may be dominated by turbule...
Gas processes affecting star formation are reviewed with an emphasis on gravitational and magnetic i...
In this work, we investigate the dynamical evolution of spherical self-gravitating systems under the...
We have analysed two cosmological zoom simulations with $M_{\rm vir}\sim 10^{12}{\rm\,M}_\odot$ from...
We use hydrodynamical simulations of galaxy clusters and groups to study the effect of pre-heating o...
The luminosity of young giant planets can inform about their formation and accretion history. The di...
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