Results 51 to 60 of about 5,089,625 (177)
After The Fall: Resolving the Molecular Gas in Post-starburst Galaxies
Abstract Post-starburst (PSB), or “E + A,” galaxies represent a rapid transitional phase between major, gas-rich mergers and gas-poor, quiescent, early-type galaxies. Surprisingly, many PSBs have been shown to host a significant interstellar medium (ISM), despite theoretical predictions that the majority of the star-forming gas should be
Adam Smercina +10 more
openaire +2 more sources
E+A galaxies represent a class of recently quenched objects, with spectra that show evidence of a previous substantial starburst and strong Balmer absorption lines indicative of A-type stellar populations.
Eric Ludwig +5 more
doaj +1 more source
Spatial Distribution of the Starbursts in Post-Starburst Coma Cluster Galaxies [PDF]
22 pages + 13 of 15 figures, uuencoded gzipped postscript.
Caldwell, N +3 more
openaire +3 more sources
Starburst Galaxies in Their Last Billion Years: An Hδ Absorption Line Selected Sample
In this paper, we focus on the study of starburst galaxies in their final billion years. Our galaxy selection is based solely on the presence of the H δ absorption line, which permits the later evolution of starburst galaxies to be traced, coinciding ...
Shumei Wu +3 more
doaj +1 more source
The Post-starburst Evolution of Tidal Disruption Event Host Galaxies [PDF]
Abstract We constrain the recent star formation histories of the host galaxies of eight optical/UV-detected tidal disruption events (TDEs). Six hosts had quick starbursts of <200 Myr duration that ended 10–1000 Myr ago, indicating that TDEs arise at different times in their hosts’ post-starburst evolution. If the disrupted star formed
K. Decker French +2 more
openaire +2 more sources
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
DESI Survey Validation Spectra Reveal an Increasing Fraction of Recently Quenched Galaxies at z ∼ 1
We utilize ∼17,000 bright luminous red galaxies (LRGs) from the novel Dark Energy Spectroscopic Instrument Survey Validation spectroscopic sample, leveraging its deep (∼2.5 hr galaxy ^−1 exposure time) spectra to characterize the contribution of recently
David J. Setton +26 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
The role of E plus A and post-starburst galaxies - II. Spectral energy distributions and comparison with observations [PDF]
In a previous paper, we have shown that the classical definition of E+A galaxies excludes a significant number of post-starburst galaxies. We suggested that analysing broad-band spectral energy distributions (SEDs) is a more comprehensive method to ...
Kotulla, R. +4 more
core +1 more source

