Results 71 to 80 of about 149 (141)
A Comparative Study of Ultraluminous Infrared Galaxies in the IRAS and SDSS Surveys
We present a comprehensive study of ultraluminous infrared galaxies (ULIRGs), leveraging data from the Infrared Astronomical Satellite Faint Source Catalogue and the spectroscopic catalog in the Sloan Digital Sky Survey Data Release 16.
Shaohua Zhang +5 more
doaj +1 more source
Extragalactic Science with the Orbiting Astronomical Satellite Investigating Stellar Systems (OASIS) Observatory. [PDF]
Aalto S +7 more
europepmc +1 more source
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
Polarized thermal emission from dust in a galaxy at redshift 2.6. [PDF]
Geach JE +7 more
europepmc +1 more source
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
Formation of Quasar Nuclei in the Hearts of Ultraluminous Infrared Galaxies
6 pages, no figure.
Taniguchi, Yoshiaki +3 more
openaire +2 more sources
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 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

