Results 91 to 100 of about 30,280 (240)

Predicting HCN, HCO + , multi-transition CO, and dust emission of star-forming galaxies. From local spiral and ultraluminous infrared galaxies to high-z star-forming and submillimeter galaxies [PDF]

open access: yes, 2016
High-z star-forming galaxies have significantly higher gas fractions and star-formation efficiencies per molecular gas mass than local star-forming galaxies.
B. Vollmer   +6 more
semanticscholar   +1 more source

Dynamics of Molecular Gas in the Central Region of the Quasar I Zwicky 1

open access: yesThe Astrophysical Journal, 2023
We present a study of the molecular gas distribution and kinematics in the cicumnuclear region (radii ≲2 kpc) of the z ≈ 0.061 quasar I Zwicky 1 using a collection of available Atacama Large Millimeter/submillimeter Array observations of the carbon ...
Qinyue Fei   +6 more
doaj   +1 more source

Millimeter-Wave Spectroscopy and Mapping of Quasar Hosts, and the Status of ULIRGs as Quasar 2s [PDF]

open access: yes, 1998
It is becoming possible to detect high redshift quasars in various molecular lines, and to show by mapping lensed objects that the strong dust and molecular emission arises in warm dense ~100 pc-scale "tori." The properties of ULIRGs, at least those with
Alloin   +54 more
core   +2 more sources

Spectropolarimetry of the ultraluminous infrared galaxy IRAS 110548–1131 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 1993
Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]
S. Young   +4 more
openaire   +1 more source

PASSAGES: The Wide-ranging, Extreme Intrinsic Properties of Planck-selected, Lensed Dusty Star-forming Galaxies

open access: yesThe Astrophysical Journal
The PASSAGES (Planck All-Sky Survey to Analyze Gravitationally-lensed Extreme Starbursts) collaboration has recently defined a sample of 30 gravitationally lensed dusty star-forming galaxies (DSFGs). These rare, submillimeter-selected objects enable high-
Patrick S. Kamieneski   +13 more
doaj   +1 more source

Starbursts in Ultraluminous Infrared Galaxies — Fueling and Properties [PDF]

open access: yes, 2001
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)
openaire   +2 more sources

ULTRALUMINOUS INFRARED GALAXIES IN THE AKARI ALL-SKY SURVEY [PDF]

open access: yes, 2014
We present a new catalog of 118 ultraluminous infrared galaxies (ULIRGs) and one hyperluminous infrared galaxy (HLIRG) by cross-matching the AKARI all-sky survey with the Sloan Digital Sky Survey Data Release 10 (SDSS DR10) and the final data release of ...
E. Eser, T. Goto, Y. Doi
semanticscholar   +1 more source

Characterizing the Molecular Gas in Infrared Bright Galaxies with CARMA

open access: yesThe Astrophysical Journal
We present the CO(1–0) maps of 28 infrared-bright galaxies from the Great Observatories All-Sky Luminous Infrared Galaxy Survey (GOALS) taken with the Combined Array for Research in Millimeter Astronomy (CARMA).
Katherine Alatalo   +22 more
doaj   +1 more source

Sub-arcsecond CO(1-0) and CO(2-1) observations of the ultraluminous infrared galaxy IRAS 10190+1322

open access: yes, 2007
We present the results of high resolution mapping of the CO(1-0) and CO(2-1) emission of the ultraluminous infrared galaxy (ULIRG) IRAS 10190+1322, with the IRAM interferometer, down to an angular resolution of ~0.3 arcsec. This object is composed of two
Braine   +22 more
core   +1 more source

Extended Star Formation in Luminous Infrared Galaxies at z ∼ 1 in the SMILES Field

open access: yesThe Astrophysical Journal
Luminous infrared galaxies (LIRGs) and ultraluminous infrared galaxies (ULIRGs) in the local Universe are highly centrally concentrated in the mid-infrared (MIR) and substantially more likely than non-(U)LIRGs to be involved in mergers.
Michael K. Florian   +7 more
doaj   +1 more source

Home - About - Disclaimer - Privacy