Results 101 to 110 of about 5,389 (174)
Hα Velocity Mapping of Ultraluminous Infrared Galaxies
We use imaging Fabry-Pec rot observations to explore the dynamical conditions in four southern ultra- luminous infrared galaxies. These galaxies all show morphological and kinematic fea- (L IR Z 1012 L _ ) tures indicative of a major merger, but they span a wide range of inferred dynamical ages: the youngest system is just past the -rst encounter ...
J. Christopher Mihos, Gregory D. Bothun
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A Comparative Study of Ultraluminous Infrared Galaxies in the IRAS and SDSS Surveys
We present a comprehensive study of ultraluminous infrared galaxies (ULIRGs), leveraging data from the Infrared Astronomical Satellite Faint Source Catalogue and the spectroscopic catalog in the Sloan Digital Sky Survey Data Release 16.
Shaohua Zhang +5 more
doaj +1 more source
It has long been thought that there is a connection between ultraluminous infrared galaxies (ULIRGs), quasars, and major mergers. Indeed, simulations show that major mergers are capable of triggering massive starbursts and quasars.
Alonso-Herrero +26 more
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Recent high resolution near infrared (HST-NICMOS) and mm-interferometric imaging have revealed dense gas and dust accretion disks in nearby ultra-luminous galactic nuclei.
Scoville, N. Z.
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Molecular Gas in the Powerful Radio Galaxies 3C~31 and 3C~264: Major or Minor Mergers?
We report the detection of $^{12}$CO~($1 \to 0$) and $^{12}$CO~($2 \to 1$) emission from the central regions ($\lesssim 5$--$10 {\rm kpc}$) of the two powerful radio galaxies 3C~31 and 3C~264.
Dinh-V-Trung, +5 more
core +1 more source
Starbursts in Ultraluminous Infrared Galaxies — Fueling and Properties [PDF]
6 pages, 3 embedded ps figures; uses svmult.cls and physprbb.sty (included); to appear in "Starburst galaxies - near and far", proceedings of the Ringberg workshop, eds. D. Lutz and L.J. Tacconi (to be published by Springer)
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The most remarkable class of high-redshift objects observed so far is extended Ly$\alpha$ emission-line blobs found in an over-density region at redshift 3.1.
Klaas U. +6 more
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Ionized Carbon in Galaxies: The [C ii] 158 μm Line as a Total Molecular Gas Mass Tracer Revisited
In this paper, we present a statistical study of the [C ii ] 158 μ m line and the CO(1−0) emission for a sample of ∼200 local and high- z (32 sources with z > 1) galaxies with very different physical conditions.
Yinghe Zhao +3 more
doaj +1 more source
Isomer-specific kinetics of the C+ + H2O reaction at the temperature of interstellar clouds. [PDF]
Yang T +7 more
europepmc +1 more source
Highlights: optical/NIR spectroscopy of ultraluminous infrared galaxies
This paper reviews the results from recent optical and near-infrared spectroscopic studies of ultraluminous infrared galaxies.
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