This paper is a numerical study of the condensation of the warm neutral medium (WNM) into cold neutral medium (CNM) structures under the effect of turbulence and thermal instability. It addresses the specific question of the CNM formation in the physical condition of the local interstellar medium (ISM). We use the properties of the H
We investigate with 3D hydrodynamical simulations the role played by thermal processes in the d...
We present 3D high resolution numerical simulations of turbulent converging interstellar atomic hyd...
Abstract. The analysis of the thermal and chemical equilibrium states of the inter-stellar medium sh...
This paper is a numerical study of the condensation of the warm neutral medium (WNM) into ...
International audienceThis paper is a numerical study of the condensation of the warm neutral medium...
Abstract. Our understanding on the physical processes in the transition between warm neutral medium ...
International audienceAims:We study in some details the statistical properties of the turbulent 2-ph...
We present a numerical and analytical study of the thermal fragmentation of a turbulent flow of inte...
The cold diffuse interstellar medium (ISM) is turbulent with supersonic, most likely transAlfvénic m...
Aims.We study in some details the statistical properties of the turbulent 2-phase interstellar atom...
{We study in some details the statistical properties of the turbulent 2-phase interstellar atomic ga...
The interstellar medium (ISM) is subject, on one hand, to heating and cooling processes that tend to...
We present a model for the development of density structure in the neutral interstellar medium. In t...
We study the thermal structure of the neutral atomic (H i) interstellar medium across a wide range o...
Context. Molecular clouds, which harbor the birthplaces of stars, form out of the atomic phase of th...
We investigate with 3D hydrodynamical simulations the role played by thermal processes in the d...
We present 3D high resolution numerical simulations of turbulent converging interstellar atomic hyd...
Abstract. The analysis of the thermal and chemical equilibrium states of the inter-stellar medium sh...
This paper is a numerical study of the condensation of the warm neutral medium (WNM) into ...
International audienceThis paper is a numerical study of the condensation of the warm neutral medium...
Abstract. Our understanding on the physical processes in the transition between warm neutral medium ...
International audienceAims:We study in some details the statistical properties of the turbulent 2-ph...
We present a numerical and analytical study of the thermal fragmentation of a turbulent flow of inte...
The cold diffuse interstellar medium (ISM) is turbulent with supersonic, most likely transAlfvénic m...
Aims.We study in some details the statistical properties of the turbulent 2-phase interstellar atom...
{We study in some details the statistical properties of the turbulent 2-phase interstellar atomic ga...
The interstellar medium (ISM) is subject, on one hand, to heating and cooling processes that tend to...
We present a model for the development of density structure in the neutral interstellar medium. In t...
We study the thermal structure of the neutral atomic (H i) interstellar medium across a wide range o...
Context. Molecular clouds, which harbor the birthplaces of stars, form out of the atomic phase of th...
We investigate with 3D hydrodynamical simulations the role played by thermal processes in the d...
We present 3D high resolution numerical simulations of turbulent converging interstellar atomic hyd...
Abstract. The analysis of the thermal and chemical equilibrium states of the inter-stellar medium sh...