The first stars: formation, properties, and impact
RS Klessen, SCO Glover - Annual Review of Astronomy and …, 2023 - annualreviews.org
The first generation of stars, often called Population III (or Pop III), form from metal-free
primordial gas at redshifts z∼ 30 and below. They dominate the cosmic star-formation …
primordial gas at redshifts z∼ 30 and below. They dominate the cosmic star-formation …
Formation of the first stars
V Bromm - Reports on Progress in Physics, 2013 - iopscience.iop.org
Understanding the formation of the first stars is one of the frontier topics in modern
astrophysics and cosmology. Their emergence signalled the end of the cosmic dark ages, a …
astrophysics and cosmology. Their emergence signalled the end of the cosmic dark ages, a …
Efficient formation of massive galaxies at cosmic dawn by feedback-free starbursts
ABSTRACT JWST observations indicate a surprising excess of luminous galaxies at z∼ 10
and above, consistent with efficient conversion of the accreted gas into stars, unlike the …
and above, consistent with efficient conversion of the accreted gas into stars, unlike the …
Simulating galaxy formation with the IllustrisTNG model
A Pillepich, V Springel, D Nelson… - Monthly Notices of …, 2018 - academic.oup.com
We introduce an updated physical model to simulate the formation and evolution of galaxies
in cosmological, large-scale gravity+ magnetohydrodynamical simulations with the moving …
in cosmological, large-scale gravity+ magnetohydrodynamical simulations with the moving …
A new class of accurate, mesh-free hydrodynamic simulation methods
PF Hopkins - Monthly Notices of the Royal Astronomical Society, 2015 - academic.oup.com
We present two new Lagrangian methods for hydrodynamics, in a systematic comparison
with moving-mesh, smoothed particle hydrodynamics (SPH), and stationary (non-moving) …
with moving-mesh, smoothed particle hydrodynamics (SPH), and stationary (non-moving) …
Turbulent cold flows gave birth to the first quasars
MA Latif, DJ Whalen, S Khochfar, NP Herrington… - Nature, 2022 - nature.com
How quasars powered by supermassive black holes formed less than a billion years after
the Big Bang is still one of the outstanding problems in astrophysics, 20 years after their …
the Big Bang is still one of the outstanding problems in astrophysics, 20 years after their …
The star formation rate of turbulent magnetized clouds: comparing theory, simulations, and observations
C Federrath, RS Klessen - The Astrophysical Journal, 2012 - iopscience.iop.org
The role of turbulence and magnetic fields is studied for star formation in molecular clouds.
We derive and compare six theoretical models for the star formation rate (SFR)—the …
We derive and compare six theoretical models for the star formation rate (SFR)—the …
The sonic scale of interstellar turbulence
Understanding the physics of turbulence is crucial for many applications, including weather,
industry and astrophysics. In the interstellar medium,, supersonic turbulence plays a crucial …
industry and astrophysics. In the interstellar medium,, supersonic turbulence plays a crucial …
Primordial star formation under the influence of far ultraviolet radiation: 1540 cosmological haloes and the stellar mass distribution
We perform a large set of cosmological simulations of early structure formation and follow
the formation and evolution of 1540 star-forming gas clouds to derive the mass distribution of …
the formation and evolution of 1540 star-forming gas clouds to derive the mass distribution of …
The mass spectrum of the first stars
H Susa, K Hasegawa, N Tominaga - The Astrophysical Journal, 2014 - iopscience.iop.org
We perform cosmological hydrodynamics simulations with non-equilibrium primordial
chemistry to obtain 59 minihalos that host first stars. The obtained minihalos are used as the …
chemistry to obtain 59 minihalos that host first stars. The obtained minihalos are used as the …