Dynamics of blue compact galaxies, as revealed by their H alpha velocity fields - II. Mass models and the starburst triggering mechanism [PDF]
Göran Östlin+5 more
openalex
Supernova dust destruction in the magnetized turbulent ISM. [PDF]
Kirchschlager F, Mattsson L, Gent FA.
europepmc +1 more source
Large turbulent reservoirs of cold molecular gas around high-redshift starburst galaxies [PDF]
Starburst galaxies at the peak of cosmic star formation are among the most extreme star-forming engines in the Universe, producing stars over about 100 million years (ref. 2).
E Falgarone, R J Ivison, Fabian Walter
exaly +2 more sources
Stellar populations dominated by massive stars in dusty starburst galaxies across cosmic time [PDF]
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, D Romano, R J Ivison
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The evolution of post-starburst galaxies from z=2 to 0.5 [PDF]
We present the evolution in the number density and stellar mass functions of photometrically selected post-starburst galaxies in the UKIDSSUltraDeep Survey,with redshifts of 0.5 10.
Vivienne Wild+2 more
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DISCOVERY OF LARGE MOLECULAR GAS RESERVOIRS IN POST-STARBURST GALAXIES [PDF]
Post-starburst (or “E+A”) galaxies are characterized by low Hα emission and strong Balmer absorption, suggesting a recent starburst, but little current star formation.
K Decker French+2 more
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Dusty starburst galaxies in the early Universe as revealed by gravitational lensing
Nature, 2013In the past decade, our understanding of galaxy evolution has been revolutionized by the discovery that luminous, dusty starburst galaxies were 1,000 times more abundant in the early Universe than at present.
J D Vieira+2 more
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A massive, cooling-flow-induced starburst in the core of a luminous cluster of galaxies
Nature, 2012In the cores of some clusters of galaxies the hot intracluster plasma is dense enough that it should cool radiatively in the cluster’s lifetime, leading to continuous ‘cooling flows’ of gas sinking towards the cluster centre, yet no such cooling flow has
M Mcdonald+2 more
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The Demographics of Starburst Galaxies
AIP Conference Proceedings, 2005With the advent of an explosion of new data on star formation rates in galaxies from SDSS, 2DF, GALEX, Spitzer, HST, and an armada of new Hα imaging surveys, we are in the midst of a revolution in our understanding of starbursts and their host galaxies.
Sanae Akiyama+4 more
openaire +2 more sources