Results 131 to 140 of about 35,402 (267)
The subarcsecond infrared structures at the centers of infrared-luminous galaxies
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
openaire +2 more sources
We report the physical properties of the 18 brightest ( S _870 _μ _m = 12.4–19.2 mJy) and not strongly lensed 870 μ m–selected dusty star-forming galaxies (DSFGs), also known as submillimeter galaxies (SMGs), in the COSMOS field.
Cheng-Lin Liao+13 more
doaj +1 more source
Progressive Starbursts and High Velocities in the Infrared-luminous, Colliding Galaxy Arp 118 [PDF]
S. A. Lamb, N. Hearn, Yu Gao
openalex +1 more source
Poststarburst galaxies are believed to be in a rapid transition between major merger starbursts and quiescent ellipticals, where active galactic nucleus (AGN) feedback is suggested as one of the processes responsible for the quenching.
Dalya Baron+4 more
doaj +1 more source
We present detailed spectral energy distribution (SED) modeling of 14 local ultraluminous infrared galaxies (ULIRGs) with outstanding photometric data from the literature covering the ultraviolet–infrared (FIR) and radio bands (∼50 MHz to ∼30 GHz).
Subhrata Dey+3 more
doaj +1 more source
Luminous Infrared Galaxies. III. Multiple Merger, Extended Massive Star Formation, Galactic Wind, and Nuclear Inflow in NGC 3256 [PDF]
S. Lípari+5 more
openalex +1 more source
Molecular Gas in Infrared-Excess, Optically Selected and the Quasars Connection with Infrared-Luminous Galaxies [PDF]
A. Evans+3 more
openalex +1 more source
Spitzer view on the evolution of star-forming galaxies from z=0 to z~3
We use a 24 micron selected sample containing more than 8,000 sources to study the evolution of star-forming galaxies in the redshift range from z=0 to z~3.
Almudena Alonso‐Herrero+25 more
core +1 more source
What powers luminous infrared galaxies?
Based on the initial data sets taken with the ISO short wavelength spectrometer (SWS) we present a first discussion of the source of luminosity of (ultra-)luminous infrared galaxies (ULIRGs). By comparison of observations of 2.5-45 mu m lines to classical starbursts and active galactic nuclei and by modelling of the line emission we show that three key
Lutz, D+10 more
openaire +2 more sources
We present JWST NIRCam imaging targeting 13 z ~ 3 infrared-luminous ( L _IR ∼ 5 × 10 ^12 L _⊙ ) galaxies from the ALESS survey with uniquely deep, high-resolution (0 $\mathop{.}\limits^{\unicode{x02033}}$ 08–0 $\mathop{.}\limits^{^{\prime\prime} }$ 16)
J. A. Hodge+27 more
doaj +1 more source