Results 51 to 60 of about 149 (141)

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

The Hosts of Ultraluminous Infrared Galaxies

open access: yes, 1999
LaTex, 6 pages with 2 embedded postscript figures and updated references; submitted to the XVth IAP Meeting "Galaxy Dynamics: from the Early Universe to the Present", Paris, France, 9-13 July ...
Sanders, D. B.   +4 more
openaire   +2 more sources

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

The JCMT SCUBA-2 Survey of the James Webb Space Telescope North Ecliptic Pole Time-Domain Field

open access: yesThe Astrophysical Journal Supplement Series, 2023
The James Webb Space Telescope Time-Domain Field (JWST-TDF) is an ∼14′ diameter field near the North Ecliptic Pole that will be targeted by one of the JWST Guaranteed Time Observations programs. Here, we describe our James Clerk Maxwell Telescope SCUBA-2
Minhee Hyun   +16 more
doaj   +1 more source

Mid-Infrared and Optical Spectroscopy of Ultraluminous Infrared Galaxies: A Comparison

open access: yesThe Astrophysical Journal, 1999
aastex, 1 eps figure. Accepted by ApJ (Letters)
Lutz, D., Veilleux, S., Genzel, R.
openaire   +2 more sources

Calibrating Mid-infrared Emission Features as Diagnostics of Star Formation in Infrared-luminous Galaxies via Radiative Transfer Modeling

open access: yesThe Astrophysical Journal
Luminous infrared (IR) galaxies are key sites of obscured stellar mass assembly at z > 0.5. Their star formation rates (SFRs) are often estimated using the luminosities of the 6.2 and 11.2 μ m polycyclic aromatic hydrocarbon (PAH) features or those of ...
Loren Robinson   +15 more
doaj   +1 more source

Star formation in the ultraluminous infrared galaxy F00183-7111 [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society: Letters, 2014
Abstract We report the detection of molecular CO(1–0) gas in F00183-7111, one of the most extreme ultraluminous infrared galaxies (ULIRGs) known, with the Australia Telescope Compact Array. We measure a redshift of 0.3292 for F00183-7111 from the CO(1–0) line and estimate the mass of the molecular gas in 00183 to be 1 × 1010 M⊙.
Mao, Minnie Y.   +7 more
openaire   +3 more sources

AChandraX‐Ray Survey of Ultraluminous Infrared Galaxies [PDF]

open access: yesThe Astrophysical Journal, 2005
40 pages, 5 tables, 14 figures, accepted by ...
Teng, SH   +5 more
openaire   +3 more sources

Direct Evidence for Active Galactic Nuclei Feedback from Fast Molecular Outflows in Reionization-era Quasars

open access: yesThe Astrophysical Journal
Galactic outflows driven by rapidly accreting quasars at high redshift are widely expected to play a key role in the short- and long-term future evolution of their host galaxies.
Justin S. Spilker   +6 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

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