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The evolution of the cold interstellar medium in galaxies following a starburst★ [PDF]
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
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Abundance diagnosis of E+A (post-starburst) galaxies [PDF]
Accepted for publication in ...
Tomotsugu Gotō
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Evolution of the cold gas properties of simulated post-starburst galaxies [PDF]
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
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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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Post-starburst galaxies in simulations and observations
2022Post-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
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The UV enigma of post-starburst galaxies
Astrophysics and Space Science, 2014We have studied the panchromatic broad-band properties from the FUV to the MIR of a sample of 808 post-starburst galaxies. We find that in the optical and near-IR bands post-starburst galaxies (PSGs) form a remarkably uniform class of objects and that, on average, simple populations synthesis models (SSP) reproduce very well the SEDs of PSGs over a ...
Melnick, J, De Propris, R
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Chemical evolution of local post-starburst galaxies: implications for the mass–metallicity relation [PDF]
We use the stellar fossil record to constrain the stellar metallicity evolution and star-formation histories of the post-starburst (PSB) regions within 45 local post-starburst galaxies from the MaNGA survey. The direct measurement of the regions' stellar
Yirui Zheng +2 more
exaly +2 more sources
Rise and fall of post-starburst galaxies in Magneticum Pathfinder
Monthly Notices of the Royal Astronomical Society, 2021Andreas Burkert +2 more
exaly
Inverse stellar population age gradients of post-starburst galaxies at z = 0.8 with LEGA-C
Monthly Notices of the Royal Astronomical Society, 2020Rachel Bezanson +2 more
exaly

