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 …
The origin of free-floating planets
N Miret-Roig - Astrophysics and Space Science, 2023 - Springer
Free-floating planets (FFPs) are the lightest products of star formation and they carry
important information on the initial conditions of the environment in which they were formed …
important information on the initial conditions of the environment in which they were formed …
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 …
Rejuvenating infall: a crucial yet overlooked source of mass and angular momentum
MHD models and the observation of accretion streamers confirmed that protostars can
undergo late accretion events after the initial collapse phase. To provide better constraints …
undergo late accretion events after the initial collapse phase. To provide better constraints …
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions–XV. Steady accretion from global collapse to core feeding in massive hub-filament …
FW Xu, K Wang, T Liu, PF Goldsmith… - Monthly Notices of …, 2023 - academic.oup.com
ABSTRACT We present ALMA Band-3/7 observations towards 'the Heart'of a massive hub-
filament system (HFS) SDC335, to investigate its fragmentation and accretion. At a …
filament system (HFS) SDC335, to investigate its fragmentation and accretion. At a …
The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). VIII. Dynamics of Embedded Dense Cores
S Li, P Sanhueza, Q Zhang, G Guido… - The Astrophysical …, 2023 - iopscience.iop.org
We present dynamical properties of 294 cores embedded in twelve IRDCs observed as part
of the ASHES Survey. Protostellar cores have higher gas masses, surface densities, column …
of the ASHES Survey. Protostellar cores have higher gas masses, surface densities, column …
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 …
ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions–XI. From inflow to infall in hub-filament systems
JW Zhou, T Liu, NJ Evans, G Garay… - Monthly Notices of …, 2022 - academic.oup.com
We investigate the presence of hub-filament systems in a large sample of 146 active proto-
clusters, using H13CO+ J= 1-0 molecular line data obtained from the ATOMS survey. We …
clusters, using H13CO+ J= 1-0 molecular line data obtained from the ATOMS survey. We …
The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). IX. Physical Properties and Spatial Distribution of Cores in IRDCs
K Morii, P Sanhueza, F Nakamura… - The Astrophysical …, 2023 - iopscience.iop.org
The initial conditions found in infrared dark clouds (IRDCs) provide insights on how high-
mass stars and stellar clusters form. We have conducted high-angular resolution and high …
mass stars and stellar clusters form. We have conducted high-angular resolution and high …