Results 21 to 30 of about 73,764 (311)
We examine the origin of molecular gas heating in a sample of 42 infrared-luminous galaxies at ...
Duncan Farrah +15 more
doaj +1 more source
Luminous infrared starbursts in a cluster of galaxies [PDF]
5 pages, 2 figures, proceedings of the IAU Colloquium 195, "Outskirts of Galaxy Clusters: intense life in the suburbs", A.
Duc, Pierre-Alain +8 more
openaire +2 more sources
GOALS-JWST: Unveiling Dusty Compact Sources in the Merging Galaxy IIZw096
We have used the Mid-InfraRed Instrument (MIRI) on the James Webb Space Telescope (JWST) to obtain the first spatially resolved, mid-infrared images of IIZw096, a merging luminous infrared galaxy (LIRG) at z = 0.036.
Hanae Inami +32 more
doaj +1 more source
Evolution of Very Luminous Infrared Galaxies [PDF]
We have completed spectroscopic observations (Wu et al. 1997a) of a sample of 73 very luminous infrared galaxies (log(LIR/L⊙) ≥ 11.5;H0 = 50 km s−1 Mpc−1) from the 2-Jy catalogue (Strauss et al. 1992) using the 2.16m telescope at the Beijing Astronomical Observatory. Spectral and interacting classifications are performed for the sample (Wu et al. 1997b)
H. Wu, Z. L. Zou, X. Y. Xia, Z. G. Deng
openaire +1 more source
The hidden heart of the luminous infrared galaxy IC 860 [PDF]
High-resolution (0.″03–0.″09 (9–26 pc)) ALMA (100–350 GHz (λ3 to 0.8 mm)) and (0.″04 (11 pc)) VLA 45 GHz measurements have been used to image continuum and spectral line emission from the inner (100 pc) region of the nearby infrared luminous galaxy
S. Aalto +21 more
semanticscholar +1 more source
We present JWST Mid-InfraRed Instrument/Medium-Resolution Spectrometer (MIRI/MRS) observations of an infrared luminous disk galaxy, FLS1, at z ∼ 0.54. With a lookback time of 5 Gyr, FLS1 is chronologically at the midpoint between the peak epoch of star ...
Jason Young +18 more
doaj +1 more source
A Near-infrared-faint, Far-infrared-luminous Dusty Galaxy at z ∼ 5 in COSMOS-Web
A growing number of far-infrared (FIR) bright sources completely invisible in deep extragalactic optical surveys hint at an elusive population of z > 4 dusty, star-forming galaxies.
Jed McKinney +34 more
doaj +1 more source
Morphological classification of local luminous infrared galaxies [PDF]
We present an analysis of the morphological classification of 89 luminous infrared galaxies (LIRGs) from the Great Observatories All-sky LIRG Survey (GOALS) sample using non-parametric coefficients and compare their morphology as a function of wavelength. We rely on images obtained in the optical (B- and I-band) as well as in the infrared (H-band and 5.
Psychogyios, A. +8 more
openaire +5 more sources
Super-Eddington Accretion in the WISE-selected Extremely Luminous Infrared Galaxy W2246−0526 [PDF]
We use optical and near-infrared spectroscopy to observe rest-UV emission lines and estimate the black hole mass of WISEA J224607.56−052634.9 (W2246−0526) at z = 4.601, the most luminous hot, dust-obscured galaxy yet discovered by WISE.
Chaowei Tsai +10 more
semanticscholar +1 more source
WARM MOLECULAR GAS IN LUMINOUS INFRARED GALAXIES [PDF]
We present our initial results on the CO rotational spectral line energy distribution (SLED) of the $J$ to $J$$-$1 transitions from $J=4$ up to $13$ from Herschel SPIRE spectroscopic observations of 65 luminous infrared galaxies (LIRGs) in the Great Observatories All-Sky LIRG Survey (GOALS).
N. Lu +20 more
openaire +3 more sources

