Results 11 to 20 of about 36,963 (210)
VIBRATIONALLY EXCITED HCN IN THE LUMINOUS INFRARED GALAXY NGC 4418 [PDF]
Infrared pumping and its effect on the excitation of HCN molecules can be important when using rotational lines of HCN to probe dense molecular gas in galaxy nuclei.
K. Sakamoto +4 more
semanticscholar +3 more sources
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
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
SOFIA/HAWC+ View of an Extremely Luminous Infrared Galaxy: WISE 1013+6112 [PDF]
We present far-infrared (FIR) properties of an extremely luminous infrared galaxy (ELIRG) at zspec = 3.703, WISE J101326.25+611220.1 (WISE 1013+6112).
Y. Toba +8 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
Arp 302: Nonstarburst Luminous Infrared Galaxies [PDF]
AAS Latex plus two postscript figures. ApJ Letters (accepted)
Lo, K. Y., Gao, Yu, Gruendl, Robert A.
openaire +2 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
JADES Imaging of GN-z11: Revealing the Morphology and Environment of a Luminous Galaxy 430 Myr after the Big Bang [PDF]
We present JWST NIRCam nine-band near-infrared imaging of the luminous z = 10.6 galaxy GN-z11 from the JWST Advanced Deep Extragalactic Survey of the GOODS-N field.
S. Tacchella +47 more
semanticscholar +1 more source
Missing Giants: Predictions on Dust-obscured Galaxy Stellar Mass Assembly Throughout Cosmic Time
Due to their extremely dust-obscured nature, much uncertainty still exists surrounding the stellar mass growth and content in dusty, star-forming galaxies (DSFGs) at z > 1. In this work, we present a numerical model built using empirical data on DSFGs to
Arianna S. Long +7 more
doaj +1 more source
Environmental dependence of local luminous infrared galaxies [PDF]
14 pages, 17 figures. To appear in A&A. Paper with high resolution figures is available at http://astro.kias.re.kr/~hshwang/doc/ms_hwang_lirg ...
Hwang, Ho Seong +6 more
openaire +2 more sources

