Results 51 to 60 of about 5,089,625 (177)

After The Fall: Resolving the Molecular Gas in Post-starburst Galaxies

open access: yesThe Astrophysical Journal, 2022
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

Comparing Star Formation Histories and Evolutionary Pathways of Post-starburst and E+A Galaxies in TNG50 and SDSS-IV MaNGA

open access: yesThe Astrophysical Journal
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]

open access: yesThe Astronomical Journal, 1996
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

open access: yesThe Astrophysical Journal
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]

open access: yesThe Astrophysical Journal, 2017
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

ADF22-WEB: Detection of a Molecular Gas Reservoir in a Massive Quiescent Galaxy Located in a z ≈ 3 Protocluster Core

open access: yesThe Astrophysical Journal Letters
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

open access: yesThe Astrophysical Journal Letters, 2023
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

open access: yesThe Astrophysical Journal
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

open access: yesThe Open Journal of Astrophysics
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]

open access: yes, 2009
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

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