Results 31 to 40 of about 232,414 (225)
Why Post-starburst Galaxies Are Now Quiescent [PDF]
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]
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]
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.
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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]
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 (
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Formaldehyde Densitometry of Starburst Galaxies [PDF]
Accepted ApJ; 16 pages, 12 figures, 7 tables, emulateapj ...
Jeremy Darling+3 more
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Rotating Starburst Cores in Massive Galaxies at z = 2.5 [PDF]
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]
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]
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]
23 pages 16 figures,2000,ApJ,545 in press.
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