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 …
The numerical frontier of the high-redshift Universe
TH Greif - Computational Astrophysics and Cosmology, 2015 - Springer
The first stars are believed to have formed a few hundred million years after the big bang in
so-called dark matter minihalos with masses∼ 10 6 M⊙ ∼10^6M_⊙. Their radiation lit up …
so-called dark matter minihalos with masses∼ 10 6 M⊙ ∼10^6M_⊙. Their radiation lit up …
[图书][B] Supernova explosions
D Branch, JC Wheeler - 2017 - Springer
JCW had long wanted to write a new monograph on supernovae. Despite an immense
explosion in the literature and many review articles, there had not been one since that of …
explosion in the literature and many review articles, there had not been one since that of …
Population III star formation in an X-ray background: III. Periodic radiative feedback and luminosity induced by elliptical orbits
We model Pop III star formation in different FUV and X-ray backgrounds, including radiation
feedback from protostars. We confirm previous results that a moderate X-ray background …
feedback from protostars. We confirm previous results that a moderate X-ray background …
Grids of stellar models with rotation – V. Models from 1.7 to 120 M⊙ at zero metallicity
Understanding the nature of the first stars is key to understanding the early Universe. With
new facilities such as James Webb Space Telescope (JWST) we may soon have the first …
new facilities such as James Webb Space Telescope (JWST) we may soon have the first …
The formation and gravitational-wave detection of massive stellar black hole binaries
K Belczynski, A Buonanno, M Cantiello… - The Astrophysical …, 2014 - iopscience.iop.org
If binaries consisting of two∼ 100 M☉ black holes exist, they would serve as extraordinarily
powerful gravitational-wave sources, detectable to redshifts of z∼ 2 with the advanced …
powerful gravitational-wave sources, detectable to redshifts of z∼ 2 with the advanced …
Population III star formation in an X-ray background–I. Critical halo mass of formation and total mass in stars
The first luminous objects forming in the universe produce radiation backgrounds in the far-
ultraviolet and X-ray bands that affect the formation of Population III stars. Using a grid of …
ultraviolet and X-ray bands that affect the formation of Population III stars. Using a grid of …
Kindling the First Stars. I. Dependence of Detectability of the First Stars with JWST on the Population III Stellar Masses
MS Bovill, M Stiavelli, AI Wiggins… - The Astrophysical …, 2024 - iopscience.iop.org
Abstract The first Population III (Pop III) stars formed out of primordial, metal-free gas, in
minihalos at z> 20, and kickstarted the cosmic processes of reionization and enrichment …
minihalos at z> 20, and kickstarted the cosmic processes of reionization and enrichment …
Two-dimensional simulations of pulsational pair-instability supernovae
Massive stars that end their lives with helium cores in the range of 35–65 M☉ are known to
produce repeated thermonuclear outbursts due to a recurring pair-instability. In some of …
produce repeated thermonuclear outbursts due to a recurring pair-instability. In some of …
Unique signatures of Population III stars in the global 21-cm signal
We investigate the effects of Population III stars on the sky-averaged 21-cm background
radiation, which traces the collective emission from all sources of ultraviolet and X-ray …
radiation, which traces the collective emission from all sources of ultraviolet and X-ray …