Results 91 to 100 of about 689 (170)
We present new James Webb Space Telescope Mid-Infrared Instrument Medium-Resolution Spectrometer observations of the nearby ultraluminous infrared galaxy F10565+2448.
Kylie Yui Dan +11 more
doaj +1 more source
Polarized thermal emission from dust in a galaxy at redshift 2.6. [PDF]
Geach JE +7 more
europepmc +1 more source
High Resolution Mid-Infrared Imaging of Ultraluminous Infrared Galaxies [PDF]
Observations of ultraluminous infrared galaxies (ULIRGs) with an achieved resolution approaching the diffraction limit in the mid-infrared from 8 to 25 μm using the Keck Telescopes are reported.
Becklin, E. E. +11 more
core
We report multifrequency Very Long Baseline Array (VLBA) observations at 2.3 and 8.4 GHz of three nearby ultraluminous infrared galaxies, identified via mid-infrared spectroscopic analyses as hosting deeply embedded active galactic nuclei (AGNs ...
Takayuki J. Hayashi +2 more
doaj +1 more source
We introduce a novel model to spectroscopically constrain the mid-infrared (MIR) extinction/attenuation curve from 3–17 μ m, using polycyclic aromatic hydrocarbon (PAH) emission drawn from an AKARI–Spitzer extragalactic cross-archival data set. Currently
Thomas S.-Y. Lai +6 more
doaj +1 more source
We report on a spectropolarimetric analysis of four southern ultraluminous infrared galaxies (ULIRGs), aimed at constraining the presence of hidden broad active galactic nucleus (AGN) lines.
Giro E +15 more
core +1 more source
We present the results of our investigations of spectrally and spatially resolved (sub)millimeter HCN-to-HCO ^+ flux ratios at J = 2–1, J = 3–2, and/or J = 4–3 in 18 nearby ( z 3 σ detections for both molecular lines) in position-position-velocity (PPV)
Masatoshi Imanishi +4 more
doaj +1 more source
HDF850.1 is the brightest submillimeter galaxy (SMG) in the Hubble Deep Field. It is known as a heavily dust-obscured star-forming galaxy embedded in an overdense environment at z = 5.18.
Fengwu Sun +30 more
doaj +1 more source
Electromagnetic counterparts to massive black-hole mergers. [PDF]
Bogdanović T, Miller MC, Blecha L.
europepmc +1 more source
We present CO(1–0) observations of 50 star-forming galaxies at 0.01 < z < 0.35, for which 3.3 μ m polycyclic aromatic hydrocarbon (PAH) emission flux or its upper limit is available.
Hyunjin Shim +14 more
doaj +1 more source

