Results 111 to 120 of about 270,460 (312)
The Astrophysical Journal Letters, 2023 We present the results of 0.″6-resolution observations of CO J = 3 − 2 line emission in 10 massive star-forming galaxies at z ∼ 2.2–2.5 with the Atacama Large Millimeter/submillimeter Array (ALMA).
Ken-ichi Tadaki +5 more
doaj +1 more source
Spatial Distribution of the Starbursts in Post-Starburst Coma Cluster Galaxies [PDF]
The Astronomical Journal, 1996 22 pages + 13 of 15 figures, uuencoded gzipped postscript.
Caldwell, N +3 more
openaire +3 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
Spectral Properties of Some IRAS Starburst Galaxies at HI 21-cm statistic study [PDF]
مجلة جامعة الانبار للعلوم الصرفة, 2012 Many research deal with physical properties of HI gas in all types of galaxies.The 21cm data analysis allows to measure spectral and radio properties for galaxies, so it allows to study physical operation that assistant in starformation. We interest here
AKRAM M. Ali
doaj +1 more source
The Schmidt Law at High Molecular Densities
, 2005 We have combined Halpha and recent high resolution CO(J=1-0) data to consider the quantitative relation between gas mass and star formation rate, or the so-called Schmidt law in nearby spiral galaxies at regions of high molecular density.
Egusa, Fumi +4 more
core +1 more source
Luminous infrared starbursts in a cluster of galaxies [PDF]
Proceedings of the International Astronomical Union, 2004 5 pages, 2 figures, proceedings of the IAU Colloquium 195, "Outskirts of Galaxy Clusters: intense life in the suburbs", A.
Duc, Pierre-Alain +8 more
openaire +2 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
Dense and Warm Molecular Gas and Warm Dust in Nearby Galaxies
, 2010 We performed 12CO(1-0), 13CO(1-0), and HCN(1-0) single-dish observations (beam size ~14"-18") toward nearby starburst and non-starburst galaxies using the Nobeyama 45 m telescope.
Kawabe, Ryohei +4 more
core +1 more source
Modelling ISO Galaxy Counts with Luminosity and Merger Rate Evolution [PDF]
, 1998 We model galaxy evolution in the 6.75 and 15 micron passbands of the ISO satellite, by combining models of galaxy evolution at optical wavelengths (which are consistent with the optical galaxy counts) with observed spectral energy distributions in the ...
Eales, Steve, Roche, Nathan
core +2 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