Early galaxy formation and its large-scale effects
Galaxy formation is at the heart of our understanding of cosmic evolution. Although there is a
consensus that galaxies emerged from the expanding matter background by gravitational …
consensus that galaxies emerged from the expanding matter background by gravitational …
Overview of the DESI legacy imaging surveys
Abstract The DESI Legacy Imaging Surveys (http://legacysurvey. org/) are a combination of
three public projects (the Dark Energy Camera Legacy Survey, the Bei**g–Arizona Sky …
three public projects (the Dark Energy Camera Legacy Survey, the Bei**g–Arizona Sky …
Enzo: An adaptive mesh refinement code for astrophysics
This paper describes the open-source code Enzo, which uses block-structured adaptive
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …
mesh refinement to provide high spatial and temporal resolution for modeling astrophysical …
Supermassive Dark Star candidates seen by JWST
The first generation of stars in the universe is yet to be observed. There are two leading
theories for those objects that mark the beginning of the cosmic dawn: hydrogen burning …
theories for those objects that mark the beginning of the cosmic dawn: hydrogen burning …
One hundred first stars: protostellar evolution and the final masses
We perform a large set of radiation hydrodynamic simulations of primordial star formation in
a fully cosmological context. Our statistical sample of 100 First Stars shows that the first …
a fully cosmological context. Our statistical sample of 100 First Stars shows that the first …
Formation of massive black holes in rapidly growing pre-galactic gas clouds
The origin of the supermassive black holes that inhabit the centres of massive galaxies
remains unclear,. Direct-collapse black holes—remnants of supermassive stars, with …
remains unclear,. Direct-collapse black holes—remnants of supermassive stars, with …
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 …
Simulations on a moving mesh: the clustered formation of population III protostars
The cosmic dark ages ended a few hundred million years after the big bang, when the first
stars began to fill the universe with new light. It has generally been argued that these stars …
stars began to fill the universe with new light. It has generally been argued that these stars …
The birth of a galaxy: primordial metal enrichment and stellar populations
By definition, Population III stars are metal-free, and their protostellar collapse is driven by
molecular hydrogen cooling in the gas phase, leading to large characteristic masses …
molecular hydrogen cooling in the gas phase, leading to large characteristic masses …