Until recently the dynamical evolution of the interstellar medium (ISM) was simu- lated using collisional ionization equilibrium (CIE) conditions. However, the ISM is a dynamical system, in which the plasma is naturally driven out of equilibrium due to atomic and dynamic processes operating on different timescales. A step forward in the field comprises a multi-fluid approach taking into account the joint thermal and dynamical evolutions of the ISM gas
Observations have suggested substantial departures from pressure equilibrium in the interstellar med...
State of the art models of the ISM use adaptive mesh refinement to capture small scale structures, b...
Recent numerical simulations of the interstellar medium driven by energy input from supernovae and s...
Until recently the dynamical evolution of the interstellar medium (ISM) was simu- lated using collis...
It is shown that a number of key observations of the Galactic ISM can be understood, if it is treate...
Abstract. The ISM, powered by SNe, is turbulent and permeated by a magnetic field (with a mean and a...
In star forming disk galaxies, matter circulation between stars and the interstellar gas, and, in pa...
In this review we critically assess numerical simulations of the interstellar medium (ISM), and argu...
The ISM, powered by SNe, is turbulent and permeated by a magnetic field (with a mean and a turbulent...
The interstellar medium (ISM) and in particular giant molecular clouds (GMCs) are complex and dynami...
It is shown that a number of key observations of the Galactic ISM can be understood, if it is treate...
We present magnetohydrodynamic (MHD) simulations of the star-forming multiphase interstellar medium ...
The interstellar medium of the Milky Way possesses a remarkable rangeof components, which have indiv...
We review recent 3D high resolution numerical HD and MHD studies of a multi-component and multi-phas...
Obtaining astrophysical information from diffuse cool, warm and hot plasmas in interstellar and inte...
Observations have suggested substantial departures from pressure equilibrium in the interstellar med...
State of the art models of the ISM use adaptive mesh refinement to capture small scale structures, b...
Recent numerical simulations of the interstellar medium driven by energy input from supernovae and s...
Until recently the dynamical evolution of the interstellar medium (ISM) was simu- lated using collis...
It is shown that a number of key observations of the Galactic ISM can be understood, if it is treate...
Abstract. The ISM, powered by SNe, is turbulent and permeated by a magnetic field (with a mean and a...
In star forming disk galaxies, matter circulation between stars and the interstellar gas, and, in pa...
In this review we critically assess numerical simulations of the interstellar medium (ISM), and argu...
The ISM, powered by SNe, is turbulent and permeated by a magnetic field (with a mean and a turbulent...
The interstellar medium (ISM) and in particular giant molecular clouds (GMCs) are complex and dynami...
It is shown that a number of key observations of the Galactic ISM can be understood, if it is treate...
We present magnetohydrodynamic (MHD) simulations of the star-forming multiphase interstellar medium ...
The interstellar medium of the Milky Way possesses a remarkable rangeof components, which have indiv...
We review recent 3D high resolution numerical HD and MHD studies of a multi-component and multi-phas...
Obtaining astrophysical information from diffuse cool, warm and hot plasmas in interstellar and inte...
Observations have suggested substantial departures from pressure equilibrium in the interstellar med...
State of the art models of the ISM use adaptive mesh refinement to capture small scale structures, b...
Recent numerical simulations of the interstellar medium driven by energy input from supernovae and s...