Results 61 to 70 of about 4,901,298 (173)
We present a study of the molecular gas reservoirs and dust contents in three quiescent galaxies (QGs) located in the core of the z = 3.09 SSA22 protocluster.
Hideki Umehata +2 more
doaj +1 more source
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
Caught in the Act of Quenching? -- A Population of Post-Starburst Ultra-Diffuse Galaxies
We report the discovery of post-starburst ultra-diffuse galaxies (UDGs), identified through spectroscopic analysis with KCWI at the Keck II Telescope. Our analysis is based on a sample of 44 candidate UDGs selected from the Systematically Measuring Ultra-
Loraine Sandoval Ascencio +5 more
doaj +1 more source
Observational and theoretical studies have long held that rapid gas consumption in starbursts is responsible for the formation of the most massive quiescent galaxies at high redshift.
David J. Setton +14 more
doaj +1 more source
The Delay Time Distribution of Tidal Disruption Events
Tidal disruption events (TDEs) can be observed when stars get too close to supermassive black holes and are torn apart and accreted. The delay time distribution of TDEs, or rate of TDEs as a function of time since a burst of star formation, can be used ...
Margaret Shepherd +8 more
doaj +1 more source
When we gaze upon the night sky into the stars in the Milky Way, it seems that the cosmos is constant, at least in the timescale of a lifetime. However, as our telescopes continued to improve, we have discovered that galaxies are instead dynamic systems,
Leung, Ho-Hin
core +1 more source
Clocking the Evolution of Post-starburst Galaxies: Methods and First Results [PDF]
Abstract Detailed modeling of the recent star formation histories (SFHs) of post-starburst (or “E+A”) galaxies is impeded by the degeneracy between the time elapsed since the starburst ended (post-burst age), the fraction of stellar mass produced in the burst (burst strength), and the burst duration.
K. Decker French +3 more
openaire +2 more sources
Measuring the star formation rate density from CNOC2 [PDF]
This thesis charts the evolution of the Universal Star Formation Rate Density (SFRD) across the redshift range 0.2 < z < 0.6, using the 2nd Canadian Network for Observational Cosmology Survey (CN0C2).
Whitaker, Richard James
core
Massive post-starburst galaxies at z > 1 are compact proto-spheroids [PDF]
We investigate the relationship between the quenching of star formation and the structural transformation of massive galaxies, using a large sample of photometrically-selected poststarburst galaxies in the UKIDSS UDS field.
Almaini, Omar +18 more
core +1 more source
No Metallicity Preference in Fast Radio Burst Host Galaxies
Fast radio bursts (FRBs) are millisecond-duration extragalactic radio transients of unknown origin, and studying their host galaxies could offer clues to constrain progenitor models.
Shotaro Yamasaki +3 more
doaj +1 more source

