Results 141 to 150 of about 182,258 (232)
The JWST EXCELS Survey: Insights into the Nature of Quenching at Cosmic Noon
We study 24 massive quiescent galaxies with $\mathrm{log}{{M}}_{* }/{{M}}_{\odot }\gt 10$ at 1
Maya Skarbinski +21 more
doaj +1 more source
We report the discovery of three faint and ultrafaint dwarf galaxies—Sculptor A, Sculptor B, and Sculptor C—in the direction of NGC 300 ( D = 2.0 Mpc), a Large Magellanic Cloud–mass galaxy.
David J. Sand +20 more
doaj +1 more source
RUBIES Spectroscopically Confirms the High Number Density of Quiescent Galaxies from 2 < z< 5
We present the number density of massive ( ${\mathrm{log}}({M}_{* }/{M}_{\odot })\gt 10.3$ ) quiescent galaxies at 2
Yunchong Zhang +23 more
doaj +1 more source
The properties of discrete X-ray sources in star-forming galaxies [PDF]
Observations of starburst galaxies have revealed a large number of point-like X-ray sources located within these systems, including active galactic nuclei (AGN), X-ray binaries (XRBs), and utraluminous X-ray sources (ULXs).
JACKSON, FLOYD,EMMANUEL
core
Massive quiescent galaxies have been identified out to z ∼ 7 in early JWST data, substantially exceeding (≳1 dex at z > 4) the number densities from most theoretical predictions. We investigate whether the number densities implied by the star formation
Yunchong Zhang +19 more
doaj +1 more source
Isolated, low-mass galaxies provide the opportunity to assess the impact of reionization on their star formation histories (SFHs) without the ambiguity of environmental processes associated with massive host galaxies.
Kristen B. W. McQuinn +14 more
doaj +1 more source
The Environmental Quenching Mechanisms of Field Dwarf Galaxies
Field dwarf galaxies not actively forming stars are relatively rare in the local Universe, but are present in cosmological hydrodynamical simulations.
José A. Benavides +4 more
doaj +1 more source
Groups, clusters and superclusters of galaxies [PDF]
Galaxies are observed in a diverse range of associations. Understanding the dynamical, statistical and clustering properties of aggregations of galaxies forms the main body of this thesis.
Moore, B, Moore, Ben
core
Restricted by event horizon suppression, tidal disruption events (TDEs) provide a unique window into otherwise hidden supermassive black holes (SMBHs) at the lower end of the mass spectrum, allowing the connection between star formation and SMBH mass to ...
Paige Ramsden +2 more
doaj +1 more source
The impact of cosmic filaments on starburst galaxies across cosmic times
Cosmological simulations suggest that various galaxy properties depend on their location within the cosmic web. Yet direct observational evidence of the dependence of star formation activity on distance to filaments remains scarce and is missing at z ≳ 1.
Jego Baptiste +19 more
doaj +1 more source

