Results 61 to 70 of about 10,116 (179)
Are E+A Galaxies Dusty-Starbursts?: VLA 20cm Radio Continuum Observation
E+A galaxies are characterized as a galaxy with strong Balmer absorption lines but without any [OII] or Halpha emission lines. Strong Balmer absorption lines indicate that E+A galaxies have experienced a starburst within the last 100 Msun yr^-1) hidden ...
Goto, Tomotsugu
core +3 more sources
Recent observations at low redshift have revealed that some post-starburst galaxies retain significant molecular gas reservoirs despite low ongoing star formation rates, challenging most theoretical predictions that rely on heating or expelling gas ...
Katherine A. Suess +14 more
doaj +1 more source
The UV properties of E+A galaxies: constraints on feedback-driven quenching of star formation [PDF]
We present the first large-scale study of E+A (post-starburst) galaxies that incorporates photometry in the ultraviolet (UV) wavelengths. We find that the starburst that creates the E+A galaxy typically takes place within the last Gyr and creates a high ...
Bekki +51 more
core +2 more sources
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
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
Post-starburst galaxies in simulations and observations
Post-starburst (PSB) galaxies are the galaxies in which star formation has recently been sharply truncated, as indicated by strong Balmer absorption lines alongside weak or absent nebular emission lines. PSBs are believed to be an important transitional state between the star- forming and quiescent populations, and could be important candidates for the
openaire +3 more sources
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
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
MOSFIRE Spectroscopy of Quiescent Galaxies at 1.5 < z < 2.5. II - Star Formation Histories and Galaxy Quenching [PDF]
We investigate the stellar populations for a sample of 24 quiescent galaxies at 1.5 < z < 2.5 using deep rest-frame optical spectra obtained with Keck MOSFIRE. By fitting templates simultaneously to the spectroscopic and photometric data, and exploring a
Belli, Sirio +2 more
core +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

