Results 11 to 20 of about 5,389 (174)
Ultraluminous Infrared Galaxies [PDF]
At luminosities above ~10^{11} L_sun, infrared galaxies become the dominant population of extragalactic objects in the local Universe (z < 0.5), being more numerous than optically selected starburst and Seyfert galaxies, and QSOs at comparable bolometric
BT Soifer +23 more
core +5 more sources
Mid Infrared Polarisation of Ultraluminous Infrared Galaxies [PDF]
The mid infrared polarisation properties of four Ultraluminous Infrared Galaxies (ULIRGs) have been investigated by broad band filter observations with the ISOCAM instrument on board the Infrared Space Observatory (ISO).
A. Efstathiou +46 more
core +4 more sources
Mid-infrared and optical spectroscopy of ultraluminous infrared galaxies: A comparison [PDF]
New tools from Infrared Space Observatory (ISO) mid-infrared spectroscopy have recently become available to determine the power sources of dust-obscured ultraluminous infrared galaxies (ULIRGs).
Aussel H. +9 more
core +3 more sources
High Resolution Mid-Infrared Imaging of Ultraluminous Infrared Galaxies [PDF]
Observations of ultraluminous infrared galaxies (ULIRGs) with an achieved resolution approaching the diffraction limit in the mid-infrared from 8 - 25 $\mu$m using the Keck Telescopes are reported.
A. J. Weinberger +15 more
core +6 more sources
The hyperluminous X‐ray source population
Abstract We have recently published a catalog of 1843 candidate ultraluminous X‐ray sources (ULXs). This is the largest catalog of ULXs to date and was built by cross‐correlating recent serendipitous source catalogs from the XMM‐Newton, Swift, and Chandra observatories with a large sample of galaxies, primarily from HyperLEDA.
A. D. A. MacKenzie +2 more
wiley +1 more source
Cosmic Sands: The Origin of Dusty, Star-forming Galaxies in the Epoch of Reionization
We present the Cosmic Sands suite of cosmological zoom-in simulations based on the simba galaxy formation model in order to study the buildup of the first massive and dusty galaxies in the early universe.
Sidney Lower +3 more
doaj +1 more source
Near-Infrared Spectra of Ultraluminous Infrared Galaxies [PDF]
Near infrared spectra with resolution R ~ 1100 in the rest wavelength range 1.8-2.2 microns have been obtained for a complete sample of 33 ultraluminous infrared galaxies. Of the 33 objects observed, 2 show evidence of a central AGN through either a broad Paschen-alpha line or emission in the 1.963 micron fine structure of [Si VI].
Murphy, Jr., T. W. +4 more
openaire +3 more sources
STELLAR POPULATIONS OF ULTRALUMINOUS INFRARED GALAXIES [PDF]
8 pages, 10 figures, 1 table.
Hou, L. G. +3 more
openaire +2 more sources
Ultraluminous Infrared Galaxies: Atlas of Near‐Infrared Images [PDF]
To appear in ApJSupp; 9 embedded figures; Complete ps copy with higher resolution figures available at http://www.stsci.edu ...
Bushouse, H A +8 more
openaire +3 more sources
Discovery of a Low-redshift Hot Dust-obscured Galaxy
We report the discovery of the hyperluminous, highly obscured active galactic nuclei (AGN) WISE J190445.04+485308.9 (W1904+4853, hereafter, L _bol ∼ 1.1 × 10 ^13 L _⊙ ) at z = 0.415.
Guodong Li +12 more
doaj +1 more source

