Star formation lies at the center of a web of processes that drive cosmic evolution:
generation of radiant energy, synthesis of elements, formation of planets, and development …

Star clusters form in dense, hierarchically collapsing gas clouds. Bulk kinetic energy is
transformed to turbulence with stars forming from cores fed by filaments. In the most compact …

Abstract The James Webb Space Telescope (JWST) discovered several luminous high-
redshift galaxy candidates with stellar masses of M*≳ 10 9 M⊙ at photometric redshifts z …

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 …

All ten LIGO/Virgo binary black hole (BH-BH) coalescences reported following the O1/O2
runs have near-zero effective spins. There are only three potential explanations for this. If the …

Gravitational-wave detections have revealed a previously unknown population of stellar
mass black holes with masses above 20 M⊙. These observations provide a new way to test …

The Close Binary Fraction of Solar-type Stars Is Strongly Anticorrelated with Metallicity -
IOPscience This site uses cookies. By continuing to use this site you agree to our use of cookies …

In the companion Paper XV of this series, we derive accurate total mass-to-light ratios within
a sphere of radius centred on the galaxy, as well as stellar (M/L) stars (with the dark matter …

The observation of quasars at very high redshift such as Pōniuā'ena is a challenge for
models of supermassive black hole (SMBH) formation. This work presents a study of SMBH …

Using a compilation of 25 studies from the literature, we investigate the evolution of the star-
forming galaxy (SFG) main sequence (MS) in stellar mass and star formation rate (SFR) out …