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FIRE-3: updated stellar evolution models, yields, and microphysics and fitting functions for applications in galaxy simulations
Increasingly, uncertainties in predictions from galaxy formation simulations (at sub-Milky
Way masses) are dominated by uncertainties in stellar evolution inputs. In this paper, we …
Way masses) are dominated by uncertainties in stellar evolution inputs. In this paper, we …
The dynamics and outcome of star formation with jets, radiation, winds, and supernovae in concert
We analyse the first giant molecular cloud (GMC) simulation to follow the formation of
individual stars and their feedback from jets, radiation, winds, and supernovae, using the …
individual stars and their feedback from jets, radiation, winds, and supernovae, using the …
Global hierarchical collapse in molecular clouds. Towards a comprehensive scenario
We present a unified description of the scenario of global hierarchical collapse (GHC). GHC
constitutes a flow regime of (non-homologous) collapses within collapses, in which all …
constitutes a flow regime of (non-homologous) collapses within collapses, in which all …
STARFORGE: Towards a comprehensive numerical model of star cluster formation and feedback
ABSTRACT We present STARFORGE (STAR FORmation in Gaseous Environments): a new
numerical framework for 3D radiation magnetohydrodynamic (MHD) simulations of star …
numerical framework for 3D radiation magnetohydrodynamic (MHD) simulations of star …
FROST-CLUSTERS–I. Hierarchical star cluster assembly boosts intermediate-mass black hole formation
A Rantala, T Naab, N Lahén - Monthly Notices of the Royal …, 2024 - academic.oup.com
Observations and high-resolution hydrodynamical simulations indicate that massive star
clusters assemble hierarchically from subclusters with a universal power-law cluster mass …
clusters assemble hierarchically from subclusters with a universal power-law cluster mass …
First predicted cosmic ray spectra, primary-to-secondary ratios, and ionization rates from MHD galaxy formation simulations
We present the first simulations evolving resolved spectra of cosmic rays (CRs) from MeV–
TeV energies (including electrons, positrons,(anti) protons, and heavier nuclei), in live …
TeV energies (including electrons, positrons,(anti) protons, and heavier nuclei), in live …
Self-consistent proto-globular cluster formation in cosmological simulations of high-redshift galaxies
We report the formation of bound star clusters in a sample of high-resolution cosmological
zoom-in simulations of z≥ 5 galaxies from the Feedback In Realistic Environments project …
zoom-in simulations of z≥ 5 galaxies from the Feedback In Realistic Environments project …
A model for the formation of stellar associations and clusters from giant molecular clouds
We present a large suite of magnetohydrodynamic simulations of turbulent, star-forming
giant molecular clouds (GMCs) with stellar feedback, extending previous work by simulating …
giant molecular clouds (GMCs) with stellar feedback, extending previous work by simulating …
Cluster assembly and the origin of mass segregation in the STARFORGE simulations
Stars form in dense, clustered environments, where feedback from newly formed stars
eventually ejects the gas, terminating star formation and leaving behind one or more star …
eventually ejects the gas, terminating star formation and leaving behind one or more star …
Radiative stellar feedback in galaxy formation: Methods and physics
Radiative feedback (RFB) from stars plays a key role in galaxies, but remains poorly
understood. We explore this using high-resolution, multifrequency radiation-hydrodynamics …
understood. We explore this using high-resolution, multifrequency radiation-hydrodynamics …