Context. The atomic-to-molecular hydrogen (H/H2) transition has been extensively studied as it controls the fraction of gas in a molecular state in an interstellar cloud. This fraction is linked to star-formation by the Schmidt–Kennicutt law. While theoretical estimates of the column density of the H
International audienceObservations of the cosmic evolution of different gas phases across time indic...
International audienceStar formation from the interstellar medium of galactic disks is a basic proce...
International audienceIn this study, we present a suite of high-resolution numerical simulations of ...
Context. The atomic-to-molecular hydrogen (H/H2) transition has been extensively studied as it contr...
International audienceContext. The atomic-to-molecular hydrogen (H/H2) transition has been extensive...
We present a study of the filamentary structure in the emission from the neutral atomic hydrogen (H
We present results from multifrequency radiative hydrodynamical chemistry simulations addressing pri...
We present a detailed description of a phenomenological H2 formation model and local star formation ...
Context. Towards the high galactic latitude sky, the far-infrared (FIR) intensity is tightly correla...
Much of the baryonic matter in the universe is in the form of H2, which includes most of the gas in ...
Context. Cosmic gas makes up about 90% of the baryonic matter in the Universe and H2 molecule is the...
We investigate how the removal of interstellar material by stellar feedback limits the efficiency of...
The hydrogen negative ion plays a crucial role in the formation of hydrogen molecules in the early u...
We derive radial and vertical distributions of HI and H2 gas densities in our Galaxy by using the te...
In this study, we present a suite of high-resolution numerical simulations of an isolated galaxy to ...
International audienceObservations of the cosmic evolution of different gas phases across time indic...
International audienceStar formation from the interstellar medium of galactic disks is a basic proce...
International audienceIn this study, we present a suite of high-resolution numerical simulations of ...
Context. The atomic-to-molecular hydrogen (H/H2) transition has been extensively studied as it contr...
International audienceContext. The atomic-to-molecular hydrogen (H/H2) transition has been extensive...
We present a study of the filamentary structure in the emission from the neutral atomic hydrogen (H
We present results from multifrequency radiative hydrodynamical chemistry simulations addressing pri...
We present a detailed description of a phenomenological H2 formation model and local star formation ...
Context. Towards the high galactic latitude sky, the far-infrared (FIR) intensity is tightly correla...
Much of the baryonic matter in the universe is in the form of H2, which includes most of the gas in ...
Context. Cosmic gas makes up about 90% of the baryonic matter in the Universe and H2 molecule is the...
We investigate how the removal of interstellar material by stellar feedback limits the efficiency of...
The hydrogen negative ion plays a crucial role in the formation of hydrogen molecules in the early u...
We derive radial and vertical distributions of HI and H2 gas densities in our Galaxy by using the te...
In this study, we present a suite of high-resolution numerical simulations of an isolated galaxy to ...
International audienceObservations of the cosmic evolution of different gas phases across time indic...
International audienceStar formation from the interstellar medium of galactic disks is a basic proce...
International audienceIn this study, we present a suite of high-resolution numerical simulations of ...
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