Results 21 to 30 of about 10,366 (216)

The star formation histories of z ∼ 1 post-starburst galaxies [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 2020
ABSTRACT We present the star formation histories of 39 galaxies with high-quality rest-frame optical spectra at 0.5 < z < 1.3 selected to have strong Balmer absorption lines and/or Balmer break, and compare to a sample of spectroscopically selected quiescent galaxies at the same redshift.
Vivienne Wild   +13 more
openalex   +8 more sources

The cold gas content of post-starburst galaxies [PDF]

open access: bronzeMonthly Notices of the Royal Astronomical Society, 2013
Post-starburst galaxies, or E+A galaxies, are characterized by optical spectra showing strong Balmer absorption lines, indicating a young stellar population, and little or no emission lines, implying no active star formation. These galaxies are interpreted as a transitional population between star-forming, disc-dominated galaxies and spheroidal ...
M. A. Zwaan   +3 more
openalex   +4 more sources

On Post-Starburst Galaxies Dominating Tidal Disruption Events [PDF]

open access: greenThe Astrophysical Journal Letters, 2019
Abstract A starburst induced by a galaxy merger may create a relatively thin central stellar disk at radius ≤100 pc. We calculate the rate of tidal disruption events (TDEs) by the inspiraling secondary supermassive black hole (SMBH) through the disk. With a small enough stellar velocity dispersion (
Renyue Cen
openalex   +4 more sources

Do post-starburst galaxies host compact molecular gas reservoirs? [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society: Letters, 2022
ABSTRACT We analysed the high-resolution (up to ∼0.2 arcsec) ALMA CO (2–1) and 1.3 mm dust continuum data of eight gas-rich post-starburst galaxies (PSBs) in the local Universe, six of which had been studied by a recent work. In contrast to this study reporting the detections of extraordinarily compact (i.e.
Fengwu Sun, Eiichi Egami
openalex   +3 more sources

GALAXIES PROBING GALAXIES: COOL HALO GAS FROM Az= 0.47 POST-STARBURST GALAXY [PDF]

open access: bronzeThe Astrophysical Journal, 2010
Submitted to ApJ. 13 pages, 5 figures, Figure 1 reduced in resolution.
Kate H. R. Rubin   +4 more
openalex   +4 more sources

Five E+A (post-starburst) galaxies as Brightest Cluster Galaxies [PDF]

open access: greenScience China Physics, Mechanics and Astronomy, 2010
8 pages, 2 figures and 1 table; A Brief Report in SCIENCE CHINA Physics, Mechanics & Astronomy (ScChG)
Feng-Shan Liu   +3 more
  +6 more sources

THE EVOLUTION OF POST-STARBURST GALAXIES FROM z ∼ 1 TO THE PRESENT [PDF]

open access: bronze, 2016
Post-starburst galaxies are in the transitional stage between blue, star-forming galaxies and red, quiescent galaxies, and therefore hold important clues for our understanding of galaxy evolution.
Petchara Pattarakijwanich   +3 more
openalex   +3 more sources

Evolution Through the Post-starburst Phase: Using Post-starburst Galaxies as Laboratories for Understanding the Processes that Drive Galaxy Evolution [PDF]

open access: bronzePublications of the Astronomical Society of the Pacific, 2021
Post-starburst (or "E+A") galaxies trace the fastest and most dramatic processes in galaxy evolution. Recent work studying the evolution of galaxies through this phase have revealed insights on how galaxies undergo structural and stellar population changes as well as the role of various feedback mechanisms.
K. Decker French
openalex   +4 more sources

The Post-starburst Evolution of Tidal Disruption Event Host Galaxies [PDF]

open access: bronzeThe 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
openalex   +4 more sources

The origins of post-starburst galaxies at z < 0.05 [PDF]

open access: greenMonthly Notices of the Royal Astronomical Society, 2018
Post-starburst galaxies can be identified via the presence of prominent Hydrogen Balmer absorption lines in their spectra. We present a comprehensive study of the origin of strong Balmer lines in a volume-limited sample of 189 galaxies with $0.019.5$ and projected axis ratio $b/a>0.32$.
M. M. Pawlik   +10 more
openalex   +7 more sources

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