Results 31 to 40 of about 232,414 (225)

Why Post-starburst Galaxies Are Now Quiescent [PDF]

open access: yesAstrophysical 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

Solving the Multimessenger Puzzle of the AGN-starburst Composite Galaxy NGC 1068 [PDF]

open access: yesAstrophysical 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

Masers in starburst galaxies [PDF]

open access: yesProceedings 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

Dust and CO emission towards the centers of normal galaxies, starburst galaxies and active galactic nuclei , I. New data and updated catalogue

open access: yes, 2007
Aims. The amount of interstellar matter in a galaxy determines its evolution, star formation rate and the activity phenomena in the nucleus. We therefore aimed at obtaining a data base of the 12 CO line and thermal dust emission within equal beamsizes ...
M. Albrecht, E. Krügel, R. Chini
semanticscholar   +1 more source

Starbursts in Isolated Galaxies? [PDF]

open access: yesAIP 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   +3 more sources

Formaldehyde Densitometry of Starburst Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2008
Accepted ApJ; 16 pages, 12 figures, 7 tables, emulateapj ...
Jeremy Darling   +3 more
openaire   +3 more sources

Rotating Starburst Cores in Massive Galaxies at z = 2.5 [PDF]

open access: yes, 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]

open access: yes, 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

The Galaxy Starburst/Main-sequence Bimodality over Five Decades in Stellar Mass at z ≈ 3–6.5 [PDF]

open access: yesAstrophysical Journal, 2021
We study the relation between stellar mass (M *) and star formation rate (SFR) for star-forming galaxies over approximately five decades in stellar mass ( 5.5≲log10(M*/M⊙)≲10.5 ) at z ≈ 3–6.5.
P. Rinaldi   +5 more
semanticscholar   +1 more source

Starbursts in Multiple Galaxy Mergers [PDF]

open access: yesThe Astrophysical Journal, 2001
23 pages 16 figures,2000,ApJ,545 in press.
openaire   +3 more sources

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