Results 1 to 10 of about 271,838 (312)

The State of the Molecular Gas in Post-starburst Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2023
The molecular gas in galaxies traces both the fuel for star formation and the processes that can enhance or suppress star formation. Observations of the molecular gas state can thus point to when and why galaxies stop forming stars.
K. Decker French   +9 more
doaj   +2 more sources

The evolutionary sequence of post-starburst galaxies [PDF]

open access: yes, 2017
© 2017 The Authors. There are multiple ways in which to select post-starburst galaxies in the literature. In this work, we present a study into how two well-used selection techniques have consequences on observable post-starburst galaxy parameters, such ...
Pimbblet, K. A.   +2 more
core   +5 more sources

The role of E+A and post-starburst galaxies – II. Spectral energy distributions and comparison with observations [PDF]

open access: green, 2009
‘The definitive version is available at www3.interscience.wiley.com '. Copyright Royal Astronomical Society. DOI: 10.1111/j.1365-2966.2009.15036.xIn a previous paper, we have shown that the classical definition of E+A galaxies excludes a significant ...
Anders   +59 more
core   +4 more sources

Stellar populations dominated by massive stars in dusty starburst galaxies across cosmic time [PDF]

open access: yesNature, 2018
All measurements of cosmic star formation must assume an initial distribution of stellar masses—the stellar initial mass function—in order to extrapolate from the star-formation rate measured for typically rare, massive stars (of more than eight solar ...
Zhi-Yu Zhang   +2 more
exaly   +2 more sources

The Evolution of Post-Starburst Galaxies from $z\sim1$ to the Present [PDF]

open access: yes, 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.
Ho, Shirley   +3 more
core   +2 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: yesPublications 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 has revealed insights on how galaxies undergo structural and stellar population ...
K. D. French
semanticscholar   +1 more source

The Compact Structures of Massive z ∼ 0.7 Post-starburst Galaxies in the SQuIGGL⃗E Sample [PDF]

open access: yes, 2022
We present structural measurements of 145 spectroscopically selected intermediate-redshift (z ∼ 0.7), massive (M ⋆ ∼ 1011 M ⊙) post-starburst galaxies from the SQuIGGL⃗E sample measured using wide-depth Hyper Suprime-Cam i-band imaging. This deep imaging
D. Setton   +11 more
semanticscholar   +1 more source

CH+(1-0) in a z~2.8 galaxy group: Probe of multi-phasic turbulent gas reservoirs [PDF]

open access: yesEPJ Web of Conferences, 2022
Starburst galaxies at redshifts z~2 to 4 are among the most intensely star-forming galaxies in the universe. The way they accrete their gas to form stars at such high rates is still a controversial issue.
Vidal-García Alba   +13 more
doaj   +1 more source

ALCHEMI: Results from the ALMA Comprehensive High-resolution Extragalactic Molecular Inventory of NGC253 [PDF]

open access: yesEPJ Web of Conferences, 2022
The star formation process in galaxies drives their evolution. The physical conditions which drive the star formation process in galaxies are studied using measurements of atomic and molecular species found in the dense has from which stars form in ...
Mangum Jeffrey G., Viti Serena
doaj   +1 more source

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

open access: yesMonthly 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 quiescent ...
V. Wild   +13 more
semanticscholar   +1 more source

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