FAR-INFRARED FINE-STRUCTURE LINE DIAGNOSTICS OF ULTRALUMINOUS INFRARED GALAXIES [PDF]
We present Herschel observations of six fine-structure lines in 25 Ultraluminous Infrared Galaxies at z<0.27. The lines, [O III]52, [N III]57, [O I]63, [N II]122, [O I]145, and [C II]158, are mostly single gaussians with widths <600 km s-1 and luminosities of 10^7 - 10^9 Solar.
Farrah, D. +18 more
openaire +7 more sources
We present detailed spectral energy distribution (SED) modeling of 14 local ultraluminous infrared galaxies (ULIRGs) with outstanding photometric data from the literature covering the ultraviolet–infrared (FIR) and radio bands (∼50 MHz to ∼30 GHz).
Subhrata Dey +3 more
doaj +2 more sources
A deficit of ultraluminous X-ray sources in luminous infrared galaxies [PDF]
We present results from a Chandra study of ultraluminous X-ray sources (ULXs) in a sample of 17 nearby (DL < 60 Mpc) luminous infrared galaxies (LIRGs), selected to have star formation rates (SFRs) in excess of 7 M⊙ yr −1 and low foreground Galactic ...
W. Luangtip +4 more
semanticscholar +4 more sources
Energetic nuclear transients in luminous and ultraluminous infrared galaxies [PDF]
Energetic nuclear outbursts have been discovered in luminous and ultraluminous infrared galaxies (U / LIRGs) at unexpectedly high rates. To investigate this population of transients, we performed a search in mid-IR data from the Wide-field Infrared ...
T. Reynolds +7 more
semanticscholar +1 more source
Galactic Winds across the Gas-rich Merger Sequence. II. Lyα Emission and Highly Ionized O vi and N v Outflows in Ultraluminous Infrared Galaxies [PDF]
This paper is the second in a series aimed at examining the gaseous environments of z ≤ 0.3 quasars and ultraluminous infrared galaxies (ULIRGs) as a function of AGN/host galaxy properties across the merger sequence.
W. Liu 刘 +5 more
semanticscholar +1 more source
Diffuse PeV neutrino emission from ultraluminous infrared galaxies [PDF]
Ultraluminous infrared galaxies (ULIRGs) are the most luminous and intense starburst galaxies in the Universe. Both their star formation rates and their gas surface mass densities are very high, implying a high supernova rate and an efficient energy ...
Hao-Ning He +4 more
openalex +3 more sources
Comprehensive Broadband X-Ray and Multiwavelength Study of Active Galactic Nuclei in 57 Local Luminous and Ultraluminous Infrared Galaxies Observed with NuSTAR and/or Swift/BAT [PDF]
We perform a systematic X-ray spectroscopic analysis of 57 local luminous and ultraluminous infrared galaxy systems (containing 84 individual galaxies) observed with the Nuclear Spectroscopic Telescope Array and/or Swift/BAT.
S. Yamada +6 more
semanticscholar +1 more source
Low gas-phase metallicities of ultraluminous infrared galaxies are a result of dust obscuration [PDF]
Optical spectroscopic measurements show that gas in dusty, starbursting galaxies known as ultraluminous infrared galaxies (ULIRGs) in the local Universe has a significantly lower metal content than that of gas in star-forming galaxies with similar masses.
N. Chartab +11 more
semanticscholar +1 more source
Radio properties of 10 nearby ultraluminous infrared galaxies with signatures of luminous buried active galactic nuclei [PDF]
We present the results of our multifrequency observations for 10 ultraluminous infrared galaxies (ULIRGs) made by the Karl G. Jansky Very Large Array at 1.4, 5.5, 9.0, and 14.0 GHz. Our sample is selected from ULIRGs whose active galactic nuclei (AGNs)
T. Hayashi, Y. Hagiwara, M. Imanishi
semanticscholar +1 more source
Classification of local ultraluminous infrared galaxies and quasars with kernel principal component analysis [PDF]
We present a new diagnostic diagram for local ultraluminous infrared galaxies (ULIRGs) and quasars, analysing particularly the Spitzer Space Telescope's Infrared Spectrograph (IRS) spectra of 102 local ULIRGs and 37 Palomar Green quasars.
E. Papaefthymiou +4 more
semanticscholar +1 more source

