Smoothed particle hydrodynamics method for fluid flows, towards industrial applications: Motivations, current state, and challenges
Abstract Smoothed Particle Hydrodynamics (SPH) is a relatively new meshless numerical
approach which has attracted significant attention in the last two decades. Compared with …
approach which has attracted significant attention in the last two decades. Compared with …
Photodissociation regions in the interstellar medium of galaxies
DJ Hollenbach, A Tielens - Reviews of Modern Physics, 1999 - APS
The interstellar medium of galaxies is the reservoir out of which stars are born and into
which stars inject newly created elements as they age. The physical properties of the …
which stars inject newly created elements as they age. The physical properties of the …
The SILCC (SImulating the LifeCycle of molecular Clouds) project–I. Chemical evolution of the supernova-driven ISM
S Walch, P Girichidis, T Naab, A Gatto… - Monthly Notices of …, 2015 - academic.oup.com
Abstract The SILCC (SImulating the Life-Cycle of molecular Clouds) project aims to self-
consistently understand the small-scale structure of the interstellar medium (ISM) and its link …
consistently understand the small-scale structure of the interstellar medium (ISM) and its link …
SILCC VI–Multiphase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionizing radiation, and cosmic rays
TE Rathjen, T Naab, P Girichidis… - Monthly Notices of …, 2021 - academic.oup.com
We present simulations of the multiphase interstellar medium (ISM) at solar neighbourhood
conditions including thermal and non-thermal ISM processes, star cluster formation, and …
conditions including thermal and non-thermal ISM processes, star cluster formation, and …
Chemical evolution of star-forming regions
▪ Abstract Recent advances in the understanding of the chemical processes that occur
during all stages of the formation of stars, from the collapse of molecular clouds to the …
during all stages of the formation of stars, from the collapse of molecular clouds to the …
Phantom: A smoothed particle hydrodynamics and magnetohydrodynamics code for astrophysics
We present Phantom, a fast, parallel, modular, and low-memory smoothed particle
hydrodynamics and magnetohydrodynamics code developed over the last decade for …
hydrodynamics and magnetohydrodynamics code developed over the last decade for …
Molecular depletion and thermal balance in dark cloud cores
PF Goldsmith - The Astrophysical Journal, 2001 - iopscience.iop.org
We analyze the effects of molecular depletion on the thermal balance of well-shielded,
quiescent dark cloud cores. Recent observations of the significant depletion of molecules …
quiescent dark cloud cores. Recent observations of the significant depletion of molecules …
The SILCC (SImulating the LifeCycle of molecular Clouds) project–II. Dynamical evolution of the supernova-driven ISM and the launching of outflows
P Girichidis, S Walch, T Naab, A Gatto… - Monthly Notices of …, 2016 - academic.oup.com
The SILCC project (SImulating the Life-Cycle of molecular Clouds) aims at a more self-
consistent understanding of the interstellar medium (ISM) on small scales and its link to …
consistent understanding of the interstellar medium (ISM) on small scales and its link to …
Modelling CO formation in the turbulent interstellar medium
We present results from high-resolution three-dimensional simulations of turbulent
interstellar gas that self-consistently follow its coupled thermal, chemical and dynamical …
interstellar gas that self-consistently follow its coupled thermal, chemical and dynamical …
SILCC–VII. Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
We present magnetohydrodynamic (MHD) simulations of the star-forming multiphase
interstellar medium (ISM) in stratified galactic patches with gas surface densities Σgas= 10 …
interstellar medium (ISM) in stratified galactic patches with gas surface densities Σgas= 10 …