Results 101 to 110 of about 233,270 (276)
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 ...
Benjamin F. Williams +9 more
openaire +4 more sources
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
Starburst-driven Starbursts in the Heart of Ultraluminous Infrared Galaxies [PDF]
The Astrophysical Journal, 1998 13 pages, 1 figure, ApJ (Letters) in ...
Yoshiaki Taniguchi +2 more
openaire +3 more sources
Dust Absorption and the Ultraviolet Luminosity Density at z ≈ 3 as Calibrated by Local Starburst Galaxies [PDF]
, 1999 We refine a technique to measure the absorption-corrected ultraviolet (UV) luminosity of starburst galaxies using rest-frame UV quantities alone and apply it to Lyman-limit U dropouts at z ≈ 3 found in the Hubble Deep Field (HDF).
G. Meurer, T. Heckman, D. Calzetti
semanticscholar +1 more source
Starburst Galaxies in Their Last Billion Years: An Hδ Absorption Line Selected Sample
The Astrophysical JournalIn this paper, we focus on the study of starburst galaxies in their final billion years. Our galaxy selection is based solely on the presence of the H δ absorption line, which permits the later evolution of starburst galaxies to be traced, coinciding ...
Shumei Wu +3 more
doaj +1 more source
Open Astronomy, 2011 Equivalent widths of spectral lines in the optical spectra of galaxies are commonly used to characterize their stellar populations and to get some insight on their evolution.
Fritz Jacopo +3 more
doaj +1 more source
ON THE STELLAR CONTENT OF THE STARBURST GALAXY IC10 [PDF]
The Astrophysical Journal, 2009 7 pages, 4 figures, 1 table.
Sanna N +19 more
openaire +6 more sources
THE DIFFUSE GAMMA-RAY FLUX ASSOCIATED WITH SUB-PEV/PEV NEUTRINOS FROM STARBURST GALAXIES [PDF]
, 2014 One attractive scenario for the excess of sub-PeV/PeV neutrinos recently reported by IceCube is that they are produced by cosmic rays in starburst galaxies colliding with the dense interstellar medium.
X. Chang, Xiang-Yu Wang
semanticscholar +1 more source
Polycyclic aromatic hydrocarbon feature deficit of starburst galaxies in the AKARI North Ecliptic Pole Deep field [PDF]
, 2014 We study the behaviour of polycyclic aromatic hydrocarbon (PAH) emission in galaxies at z = 0.3–1.4 using 1868 samples from the revised catalogue of AKARI North Ecliptic Pole Deep survey.
K. Murata +8 more
semanticscholar +1 more source
The Astrophysical Journal, 1992 The use of SO and SO2 as probes of the dense interstellar medium in the nearby starburst galaxies NGC 253 and M82 is described. Emission in the 99.3 GHz 3(2) - 2(1) rotational transition of SO was detected in NGC 253 and possibly in M82, and upper limits are reported for emission in the 219.9 GHz 6(5) - 5(4) transition of SO and two lines of SO2.
Charles L. Bennett, S. J. Petuchowski
openaire +2 more sources