Results 41 to 50 of about 270,460 (312)
The role of E+A and post-starburst galaxies – I. Models and model results [PDF]
, 2009 ‘The definitive version is available at www3.interscience.wiley.com '. Copyright Royal Astronomical Society. DOI: 10.1111/j.1365-2966.2009.14416.xDifferent compositions of galaxy types in the field in comparison to galaxy clusters as described by the ...
Falkenberg, M.A. +2 more
core +2 more sources
Masers in starburst galaxies [PDF]
Proceedings of the International Astronomical Union, 2007 AbstractMasers in starburst galaxies are outstanding probes of a range of phenomena related to galaxy and black hole evolution, and offer unique high brightness temperature illumination that can be used to probe small scales in the host galaxy and in our own.
openaire +2 more sources
Why Post-starburst Galaxies Are Now Quiescent [PDF]
Astrophysical Journal, 2018 Post-starburst or “E + A” galaxies are rapidly transitioning from star-forming to quiescence. While the current star formation rate (SFR) of post-starbursts is already at the level of early-type galaxies, we recently discovered that many have large CO ...
K. D. French +13 more
semanticscholar +1 more source
After the Fall: The Dust and Gas in E+A Post-starburst Galaxies [PDF]
, 2018 The traditional picture of post-starburst galaxies as dust- and gas-poor merger remnants, rapidly transitioning to quiescence, has been recently challenged.
A. Smercina +16 more
semanticscholar +1 more source
Evolution of the cold gas properties of simulated post-starburst galaxies [PDF]
Monthly notices of the Royal Astronomical Society, 2018 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
T. Davis +5 more
semanticscholar +1 more source
Starbursts in Isolated Galaxies? [PDF]
AIP Conference Proceedings, 2005 I investigated the evolution of star forming dwarf galaxies by means of a one-zone model extended for dynamical evolution. This allows for a coupling between the dynamical state of the galaxy and its internal properties like star formation activity or the thermal state of the interstellar medium (ISM). The presented work focusses on the star formation (
openaire +2 more sources
Efficient formation of massive galaxies at cosmic dawn by feedback-free starbursts [PDF]
Monthly notices of the Royal Astronomical Society, 2023 JWST observations indicate a surprising excess of luminous galaxies at z ∼ 10 and above, consistent with efficient conversion of the accreted gas into stars, unlike the suppression of star formation by feedback at later times.
A. Dekel +4 more
semanticscholar +1 more source
Odessa Astronomical Publications, 2017 Here we present observational evidences and theoretical approaches to the starburst phenomena in the different types of the galaxies. A starburst model for AGN, large-scale gas outflow of the central regions of galaxies, and ultimate fate of a matter ...
S. A. Silich
doaj +1 more source
THE NATURE OF STARBURSTS. II. THE DURATION OF STARBURSTS IN DWARF GALAXIES [PDF]
The Astrophysical Journal, 2010 The starburst phenomenon can shape the evolution of the host galaxy and the surrounding intergalactic medium. The extent of the evolutionary impact is partly determined by the duration of the starburst, which has a direct correlation with both the amount of stellar feedback and the development of galactic winds, particularly for smaller mass dwarf ...
McQuinn, Kristen B. W. +9 more
openaire +2 more sources
Integrated field spectroscopy of E+A (post-starburst) galaxies with the Kyoto3DII [PDF]
, 2008 We have performed a two-dimensional spectroscopy of three nearby E+A (post-starburst) galaxies with the Kyoto3DII integral field spectrograph. In all the cases, Hdelta absorption is stronger at the centre of the galaxies, but significantly extended in a ...
Goto, Tomotsugu +5 more
core +1 more source