Characterizing the Molecular Gas in Infrared Bright Galaxies with CARMA
The Astrophysical JournalWe 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 Astrophysical JournalWe use the CN/CO intensity ratio to obtain the dense gas fraction, f _dense , for a sample of 16 ultraluminous and luminous infrared (IR) galaxies and compare f _dense with a suite of global galaxy properties.
Blake Ledger +4 more
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Erratum: “Molecular Gas in Infrared-Excess, Optically Selected Quasars and the Connection with Infrared-luminous Galaxies” [Astron. J. [BF]121[/BF], 1893 (2001)] [PDF]
, 2001 A. Evans +3 more
openalex +2 more sources
An X‐Ray and Optical Investigation of the Infrared‐luminous Galaxy Merger Markarian 266 [PDF]
, 1997 Jing Wang +3 more
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NICMOS observations of luminous & ultraluminous infrared galaxies [PDF]
Astrophysics and Space Science, 1999 HST NICMOS observations of a sample of 24 luminous (LIGs: LIR[8-1000 μm] = 1011.0-11.99 L⊙) and ultraluminous (ULIGs:LIR ≳ 1012.0 L⊙) infrared galaxies are presented.The observations provide, for the first time, high resolution HST imagingof the imbedded 1.1 - 2.2 μm nuclear regions of these mergers.
openaire +4 more sources
Shockingly Effective: Cluster Winds as Engines of Feedback in Starburst Galaxy VV 114
The Astrophysical JournalWe present high-resolution Keck Cosmic Web Imager and MUSE integral field unit spectroscopy of VV 114, a local IR-luminous merger undergoing a vigorous starburst and showing evidence of galactic-scale feedback. The high-resolution data allow for spectral
Justin A. Kader +31 more
doaj +1 more source
Progressive Starbursts and High Velocities in the Infrared-luminous, Colliding Galaxy Arp 118 [PDF]
, 1998 S. A. Lamb, N. Hearn, Yu Gao
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The subarcsecond infrared structures at the centers of infrared-luminous galaxies
The Astrophysical Journal, 1990 This paper presents 1.6-2.2-micron imaging observations of the centers of nine galaxies with high 60-100-micron luminosities. Eight of the nine galaxies contain central 2.2-micron sources that are larger than the point spread function, which typically had a size (FWHM) of 1.0 arcsec. The typical physical size of the 2.2-micron sources is about 0.5 kpc.
C. G. Wynn-Williams +4 more
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86th Annual Meeting of the Meteoritical Society (2024)
Meteoritics &Planetary Science, Volume 59, Issue S1, Page A1-A468, August 2024.
wiley +1 more source
Searching for Low-redshift Hot Dust-obscured Galaxies
The Astrophysical JournalHot dust-obscured galaxies (Hot DOGs), discovered by the “W1W2 dropout” selection at high redshifts ( z ∼ 2–4), are a rare population of hyperluminous obscured quasars.
Guodong Li +15 more
doaj +1 more source