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 …
Cloud–cloud collisions and triggered star formation
Star formation is a fundamental process for galactic evolution. One issue over the last
several decades has been determining whether star formation is induced by external …
several decades has been determining whether star formation is induced by external …
Synthetic observations of star formation and the interstellar medium
Synthetic observations are playing an increasingly important role across astrophysics, both
for interpreting real observations and also for making meaningful predictions from models. In …
for interpreting real observations and also for making meaningful predictions from models. In …
Radiation transport methods in star formation simulations
R Wünsch - Frontiers in Astronomy and Space Sciences, 2024 - frontiersin.org
Radiation transport plays a crucial role in star formation models, as certain questions within
this field cannot be accurately addressed without taking it into account. Given the high …
this field cannot be accurately addressed without taking it into account. Given the high …
Efficient early stellar feedback can suppress galactic outflows by reducing supernova clustering
We present a novel set of stellar feedback models, implemented in the moving-mesh code
arepo, designed for galaxy formation simulations with near-parsec (or better) resolution …
arepo, designed for galaxy formation simulations with near-parsec (or better) resolution …
Which feedback mechanisms dominate in the high-pressure environment of the Central Molecular Zone?
Supernovae (SNe) dominate the energy and momentum budget of stellar feedback, but the
efficiency with which they couple to the interstellar medium (ISM) depends strongly on how …
efficiency with which they couple to the interstellar medium (ISM) depends strongly on how …
The GRIFFIN Project—Formation of Star Clusters with Individual Massive Stars in a Simulated Dwarf Galaxy Starburst
N Lahén, T Naab, PH Johansson… - The Astrophysical …, 2020 - iopscience.iop.org
We describe a population of young star clusters (SCs) formed in a hydrodynamical
simulation of a gas-rich dwarf galaxy merger resolved with individual massive stars at …
simulation of a gas-rich dwarf galaxy merger resolved with individual massive stars at …
First hydrodynamics simulations of radiation forces and photoionization feedback in massive star formation
Aims. We present the first simulations of the formation and feedback of massive stars which
account for radiation forces as well as photoionization feedback (along with protostellar …
account for radiation forces as well as photoionization feedback (along with protostellar …
Variable interstellar radiation fields in simulated dwarf galaxies: supernovae versus photoelectric heating
We present high-resolution hydrodynamical simulations of isolated dwarf galaxies including
self-gravity, non-equilibrium cooling and chemistry, interstellar radiation fields (ISRF) and …
self-gravity, non-equilibrium cooling and chemistry, interstellar radiation fields (ISRF) and …
Starbursts in low-mass haloes at Cosmic Dawn. I. The critical halo mass for star formation
The first stars, galaxies, star clusters, and direct-collapse black holes are expected to have
formed in low-mass (∼ 105–109 M⊙) haloes at Cosmic Dawn (z∼ 10–30) under conditions …
formed in low-mass (∼ 105–109 M⊙) haloes at Cosmic Dawn (z∼ 10–30) under conditions …