No Galaxy-scale [C ii] Fast Outflow in the z = 6.72 Red Quasar HSC J1205–0000
HSC 120505.09-000027.9 (J1205–0000) is one of the highest redshift ( z = 6.72) dust-reddened quasars (red quasars) known to date. We present an improved analysis of Atacama Large Millimeter/submillimeter Array data of the [C ii ] 158 μ m line and the ...
Mahoshi Sawamura+19 more
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Jet reorientation in active galactic nuclei: two winged radio galaxies [PDF]
J. Dennett-Thorpe+5 more
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FRAMEx. V. Radio Spectral Shape at Central Subparsec Region of Active Galactic Nuclei
We present results from the Very Long Baseline Array multifrequency (1.6, 4.4, 8.6, and 22 GHz), high-sensitivity (∼25 μ Jy beam ^−1 ), subparsec-scale (
Onic I. Shuvo+6 more
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Powerful Radio-loud Quasars Are Triggered by Galaxy Mergers in the Cosmic Bright Ages
While supermassive black holes are ubiquitous features of galactic nuclei, only a small minority are observed during episodes of luminous accretion. The physical mechanism(s) driving the onset of fueling and ignition in these active galactic nuclei (AGN)
Peter Breiding+17 more
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X-ray properties of coronal emission in radio quiet active galactic nuclei
Active galactic nuclei (AGN) are powerful sources of panchromatic radiation. All AGN emit in X-rays, contributing around 5%–10% of the AGN bolometric luminosity.
Sibasish Laha+11 more
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Relation between radio core length and black hole mass for active galactic nuclei [PDF]
Xinwu Cao, Dongrong Jiang
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Testing of Inverse Compton Models for Active Galactic Nuclei with Gamma‐Ray and Radio Observations [PDF]
A. Lähteenmäki, E. Valtaoja
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A Dichotomy in the 1–24 GHz Parsec-scale Radio Spectra of Radio-quiet Quasars
We present the parsec-scale radio spectra of a representative sample of 13 Palomar–Green radio-quiet quasars, based on our new Very Long Baseline Array (VLBA) observations at 8.4 and 23.6 GHz and our earlier VLBA studies at 1.5 and 5.0 GHz.
Sina Chen+5 more
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Radio-loud Active Galactic Nuclei in the Context of the Eigenvector 1 Parameter Space [PDF]
J. W. Sulentic+5 more
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Prospects of Detecting a Jet in Sagittarius A* with Very-long-baseline Interferometry
Event Horizon Telescope (EHT) images of the horizon-scale emission around the Galactic center supermassive black hole Sagittarius A* (Sgr A*) favor accretion flow models with a jet component. However, this jet has not been conclusively detected.
Erandi Chavez+5 more
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