Results 21 to 30 of about 234,875 (165)
Solving the Multimessenger Puzzle of the AGN-starburst Composite Galaxy NGC 1068 [PDF]
Astrophysical Journal, 2022 Multiwavelength observations indicate that some starburst galaxies show a dominant nonthermal contribution from their central region. These active galactic nuclei (AGN)-starburst composites are of special interest, as both phenomena on their own are ...
B. Eichmann +4 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
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
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
Rotating Starburst Cores in Massive Galaxies at z = 2.5 [PDF]
, 2017 We present spatially resolved ALMA observations of the CO emission line in two massive galaxies at z = 2.5 on the star-forming main sequence. Both galaxies have compact dusty star-forming cores with effective radii of and in the 870 μm continuum emission.
K. Tadaki +23 more
semanticscholar +1 more source
Massive post-starburst galaxies at z > 1 are compact proto-spheroids [PDF]
, 2017 We investigate the relationship between the quenching of star formation and the structural transformation of massive galaxies, using a large sample of photometrically-selected poststarburst galaxies in the UKIDSS UDS field.
O. Almaini +8 more
semanticscholar +1 more source
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
The evolution of post-starburst galaxies from z=2 to 0.5 [PDF]
, 2016 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.
V. Wild +10 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
Methods for identifying high‐redshift galaxy cluster candidates
Astronomische Nachrichten, Volume 340, Issue 7, Page 618-621, August 2019., 2019 Abstract Recent theories linked long gamma ray bursts (GRBs) to galaxies with rapid star formation or starburst; thus, we expect that long GRBs (LGRBs) are more frequent in midcluster galaxies where mergers and tidal interactions between gas‐rich galaxies are more likely to occur. Yet there is no galaxy cluster known to be associated with LGRBs.
Sandor Pinter +5 more
wiley +1 more source