Results 151 to 160 of about 4,901,298 (173)
Post-starburst galaxies in SDSS-IV MaNGA [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 Funding: European Research Council via the award of a starting grant (SEDMorph; P.I. V. Wild) (VW, KR).Post-starburst galaxies, identified by their unusually strong Balmer absorption lines and weaker than average emission lines, have traditionally been ...
Lihwai Lin +2 more
exaly +9 more sources
Post-starburst properties of post-merger galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2023 Post-starburst galaxies (PSBs) are transition galaxies showing evidence of recent rapid star formation quenching. To understand the role of galaxy mergers in triggering quenching, we investigate the incidence of PSBs and resolved PSB properties in post ...
Kate Rowlands +2 more
exaly +4 more sources
The star formation histories of z ∼ 1 post-starburst galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2020 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 ...
Kate Rowlands +2 more
exaly +4 more sources
Post-starburst quasars: bridging the gap between post-starburst galaxies and quasars [PDF]
Monthly Notices of the Royal Astronomical Society, 2015 13 pages, 9 figures, accepted for publication to ...
Michael Brotherton
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The merger fraction of post-starburst galaxies in UNIONS
Monthly Notices of the Royal Astronomical Society, 2022 ABSTRACT Post-starburst galaxies (PSBs) are defined as having experienced a recent burst of star formation, followed by a prompt truncation in further activity. Identifying the mechanism(s) causing a galaxy to experience a post-starburst phase therefore provides integral insight into the causes of rapid quenching.
Stephen Gwyn +2 more
exaly +5 more sources
Evolution of the cold gas properties of simulated post-starburst galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2019 Post-starburst galaxies are typically considered to be a transition population, en route to the red sequence after a recent quenching event. Despite this, recent observations have shown that these objects typically have large reservoirs of cold molecular
Robert A Crain +2 more
exaly +2 more sources
Abundance diagnosis of E+A (post-starburst) galaxies [PDF]
Monthly Notices of the Royal Astronomical Society, 2007 Accepted for publication in ...
Tomotsugu Gotō
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The evolution of the cold interstellar medium in galaxies following a starburst★ [PDF]
Monthly Notices of the Royal Astronomical Society, 2015 VW and KR acknowledge support from the European Research Council Starting Grant SEDmorph (P.I. VW).We present the evolution of dust and molecular gas properties in a sample of 11 z ˜ 0.03 starburst to post-starburst (PSB) galaxies selected to span an age
Kate Rowlands +2 more
exaly +2 more sources
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Astrophysics and Space Science, 1994
Observations of nearby star-forming regions suggest that the initial mass function is deficient in low-mass stars when the ambient star formation rate is high. We investigate the consequences of a truncated initial mass function on the photometric evolution of star burst galaxies using new models of stellar population synthesis. A major prediction with
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Observations of nearby star-forming regions suggest that the initial mass function is deficient in low-mass stars when the ambient star formation rate is high. We investigate the consequences of a truncated initial mass function on the photometric evolution of star burst galaxies using new models of stellar population synthesis. A major prediction with
openaire +1 more source
Post-starburst galaxies in different environments
Proceedings of the International Astronomical Union, 2019AbstractPost-starburst galaxies (PSBGs) are systems that experienced a burst followed by a rapid quenching of star formation. However, it is still unclear what causes these events and what is the environmental role in the origin of PSBGs. To address this, we analysed sizes, morphologies, ages, and metallicities of PSBGs at 0.05 ≤ z ≤ 0.1 in groups and ...
Rodolfo Spindler +2 more
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