The differential magnification of high-redshift ultraluminous infrared galaxies [PDF]
A. W. Blain
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A new look at local ultraluminous infrared galaxies: the atlas and radiative transfer models of their complex physics [PDF]
A. Efstathiou +13 more
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High-redshift star formation in the Atacama large millimetre/submillimetre array era. [PDF]
Hodge JA, da Cunha E.
europepmc +1 more source
Local Ultraluminous Infrared Galaxies and Quasars
This paper reviews the recent results from a comprehensive investigation of the most luminous mergers in the local universe, the ultraluminous infrared galaxies (ULIRGs) and the quasars. First, the frequency of occurrence and importance of black hole driven nuclear activity in ULIRGs are discussed using the latest sets of optical, near-infrared, mid ...
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Determining the inner structure of the molecular torus around an active galactic nucleus is essential for understanding its formation mechanism. However, spatially resolving the torus is difficult because of its small size.
Shusuke Onishi +8 more
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The Magnetic Fields of the Dusty Nuclei and Molecular Outflows of Arp 220
Galaxy mergers trigger starburst activity and galactic outflows that enrich the circumgalactic medium (CGM), profoundly impacting galaxy evolution. These phenomena are intrinsically linked to the physical conditions of the medium, which is permeated by ...
Enrique Lopez-Rodriguez +7 more
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Strong Evidence for a Buried Active Galactic Nucleus in UGC 5101: Implications for LINER-type Ultraluminous Infrared Galaxies [PDF]
Masatoshi Imanishi +2 more
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Disclosing Submillimeter Galaxy Formation: Mergers or Secular Evolution?
We analyze the morphology of 125 submillimeter galaxies (SMGs) in the PRIMER-COSMOS field using double Sérsic modeling on JWST NIRCam images across six bands (F150W, F200W, F277W, F356W, F410M, and F444W), with SMGs being classified by the bulge Sérsic ...
Siu-Wang Chan, Yiping Ao, Qing-hua Tan
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THE FIRST DETECTION OF GeV EMISSION FROM AN ULTRALUMINOUS INFRARED GALAXY: Arp 220 AS SEEN WITH THE FERMI LARGE AREA TELESCOPE [PDF]
Fang‐Kun Peng +4 more
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Spitzer Mid-Infrared Imaging of Nearby Ultraluminous Infrared Galaxies
We have observed 14 nearby (z<0.16) Ultraluminous Infrared Galaxies (ULIRGs) with Spitzer at 3.6-24 microns. The underlying host galaxies are well-detected, in addition to the luminous nuclear cores. While the spatial resolution of Spitzer is poor, the great sensitivity of the data reveals the underlying galaxy merger remnant, and provides the first
Surace, J. A. +6 more
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