The origin and evolution of multiple star systems
SSR Offner, M Moe, KM Kratter, SI Sadavoy… - arXiv preprint arXiv …, 2022 - arxiv.org
Observational advances over the last decade have enabled high-resolution, interferometric
studies of forming multiple systems, statistical surveys of multiplicity in star-forming regions …
studies of forming multiple systems, statistical surveys of multiplicity in star-forming regions …
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 …
FIRE-3: updated stellar evolution models, yields, and microphysics and fitting functions for applications in galaxy simulations
PF Hopkins, A Wetzel, C Wheeler… - Monthly Notices of …, 2023 - academic.oup.com
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 …
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 …
Magnetohydrodynamical modeling of star-disk formation: from isolated spherical collapse towards incorporation of external dynamics
M Kuffmeier - Frontiers in Astronomy and Space Sciences, 2024 - frontiersin.org
The formation of protostars and their disks has been understood as the result of the
gravitational collapse phase of an accumulation of dense gas that determines the mass …
gravitational collapse phase of an accumulation of dense gas that determines the mass …
Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations
One of the key mysteries of star formation is the origin of the stellar initial mass function
(IMF). The IMF is observed to be nearly universal in the Milky Way and its satellites, and …
(IMF). The IMF is observed to be nearly universal in the Milky Way and its satellites, and …
Evidence of high-mass star formation through multiscale mass accretion in hub-filament-system clouds
We present a statistical study of a sample of 17 hub-filament-system (HFS) clouds of high-
mass star formation using high-angular resolution (∼ 1–2 arcsec) ALMA 1.3 and 3 mm …
mass star formation using high-angular resolution (∼ 1–2 arcsec) ALMA 1.3 and 3 mm …
A model for the formation of stellar associations and clusters from giant molecular clouds
MY Grudić, JM Diederik Kruijssen… - Monthly Notices of …, 2021 - academic.oup.com
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 …
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 …
The Evolution of Protostellar Outflow Cavities, Kinematics, and Angular Distribution of Momentum and Energy in Orion A: Evidence for Dynamical Cores
Abstract We present Atacama Large Millimeter/submillimeter Array observations of the∼
10,000 au environment surrounding 21 protostars in the Orion A molecular cloud tracing …
10,000 au environment surrounding 21 protostars in the Orion A molecular cloud tracing …