The assembly of the first massive black holes

K Inayoshi, E Visbal, Z Haiman - Annual Review of Astronomy …, 2020 - annualreviews.org
The existence of∼ 109M⊙ supermassive black holes (SMBHs) within the first billion years
of the Universe has stimulated numerous ideas for the prompt formation and rapid growth of …

Formation of the first stars and black holes

L Haemmerlé, L Mayer, RS Klessen, T Hosokawa… - Space Science …, 2020 - Springer
We review the current status of knowledge concerning the early phases of star formation
during cosmic dawn. This includes the first generations of stars forming in the lowest mass …

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 …

Modeling the radio background from the first black holes at cosmic dawn: implications for the 21 cm absorption amplitude

A Ewall-Wice, TC Chang, J Lazio, O Doré… - The Astrophysical …, 2018 - iopscience.iop.org
We estimate the 21 cm radio background from accretion onto the first intermediate-mass
black holes between z≈ 30 and z≈ 16. Combining potentially optimistic, but plausible …

Formation of massive black holes in rapidly growing pre-galactic gas clouds

JH Wise, JA Regan, BW O'Shea, ML Norman… - Nature, 2019 - nature.com
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 …

Titans of the early Universe: The Prato statement on the origin of the first supermassive black holes

TE Woods, B Agarwal, V Bromm, A Bunker… - Publications of the …, 2019 - cambridge.org
In recent years, the discovery of massive quasars at has provided a striking challenge to our
understanding of the origin and growth of supermassive black holes in the early Universe …

Black hole mass scaling relations for early-type galaxies. I. MBH–M*, sph and MBH–M*, gal

N Sahu, AW Graham, BL Davis - The Astrophysical Journal, 2019 - iopscience.iop.org
Analyzing a sample of 84 early-type galaxies (ETGs) with directly measured supermassive
black hole masses—nearly doubling the sample size of such galaxies with multicomponent …

Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). VI. Black hole mass measurements of six quasars at 6.1≤ z≤ 6.7

M Onoue, N Kashikawa, Y Matsuoka… - The Astrophysical …, 2019 - iopscience.iop.org
We present deep near-infrared spectroscopy of six quasars at 6.1≤ z≤ 6.7 with Very Large
Telescope/X-Shooter and Gemini-N/GNIRS. Our objects, originally discovered through a …

Cradles of the first stars: self-shielding, halo masses, and multiplicity

D Skinner, JH Wise - Monthly Notices of the Royal Astronomical …, 2020 - academic.oup.com
The formation of Population III (Pop III) stars is a critical step in the evolution of the early
Universe. To understand how these stars affected their metal-enriched descendants, the …

The influence of streaming velocities and Lyman–Werner radiation on the formation of the first stars

ATP Schauer, SCO Glover, RS Klessen… - Monthly Notices of the …, 2021 - academic.oup.com
The first stars in the Universe, the so-called Population III stars, form in small dark matter
minihaloes with virial temperatures T vir< 104 K. Cooling in these minihaloes is dominated …