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101
The nature of luminous X-ray sources with mid-infrared counterparts
Published 2004“…Only about one-quarter of the hard X-ray/24 μm sources show pure type 1 active galactic nucleus (AGN) SEDs. More than half of the X-ray/24 μm sources have stellar emission-dominated or obscured SEDs, similar to those of local type 2 AGN and spiral/starburst galaxies. …”
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102
MODELING THE Fe K LINE PROFILES IN TYPE I ACTIVE GALACTIC NUCLEI WITH A COMPTON-THICK DISK WIND
Published 2012“…The sources in this sample all contain moderately broad components of FeK-shell emission and are ideal candidates for testing the applicability of a Compton-thick accretion disk wind model to active galactic nucleus (AGN) emission components. Viewing angles through the wind allow the observer to see the absorption signature of the gas, whereas face-on viewing angles allow the observer to see the scattered light from the wind. …”
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103
AGN STORM 2. I. First results: A Change in the Weather of Mrk 817
Published 2022“…<jats:title>Abstract</jats:title> <jats:p>We present the first results from the ongoing, intensive, multiwavelength monitoring program of the luminous Seyfert 1 galaxy Mrk 817. While this active galactic nucleus was, in part, selected for its historically unobscured nature, we discovered that the X-ray spectrum is highly absorbed, and there are new blueshifted, broad, and narrow UV absorption lines, which suggest that a dust-free, ionized obscurer located at the inner broad-line region partially covers the central source. …”
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104
Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter
Published 2010“…The anisotropy was measured by the fraction of arrival directions that are less than $3.1^\circ$ from the position of an active galactic nucleus within 75 Mpc (using the V\'eron-Cetty and V\'eron $12^{\rm th}$ catalog). …”
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105
Obscured activity: AGN, quasars, starbursts and uligs observed by the infrared space observatory
Published 2005“…ISO surveyed a wide range of active galaxies which, in the context of this review, includes those powered by intense bursts of star formation as well as those containing a dominant active galactic nucleus (AGN). Mid-infrared imaging resolved for the first time the dust enshrouded nuclei in many nearby galaxies, while a new era in infrared spectroscopy was opened by probing a wealth of atomic, ionic and molecular lines as well as broad band features in the mid-and farinfrared. …”
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106
Evolution of interstellar medium, star formation, and accretion at high redshift
Published 2017“…The cosmic evolution of total ISM mass is estimated and linked to the evolution of SF and active galactic nucleus activity at early epochs.…”
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107
2D kinematics and physical properties of z similar to 3 star-forming galaxies
Published 2010“…We discovered that the nearby galaxy, VVDS-020297772 (which shows traces of active galactic nucleus activity), is in fact a companion at a similar redshift with a projected separation of 12 kpc. …”
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108
H I absorption in nearby compact radio galaxies
Published 2017“…H I absorption studies yield information on both active galactic nucleus (AGN) feeding and feedback processes. …”
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109
Bubble-driven gas uplift in galaxy clusters and its velocity features
Published 2022“…Buoyant bubbles of relativistic plasma are essential for active galactic nucleus feedback in galaxy clusters, stirring and heating the intracluster medium (ICM). …”
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110
Electromagnetic Counterparts Powered by Kicked Remnants of Black Hole Binary Mergers in AGN Disks
Published 2024-01-01“…The disk of an active galactic nucleus (AGN) is widely regarded as a prominent formation channel of binary black hole (BBH) mergers that can be detected through gravitational waves (GWs). …”
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111
No Small-scale Radio Jets Here: Multiepoch Observations of Radio Continuum Structures in NGC 1068 with the VLBA
Published 2023-01-01“…We suggest that the most likely explanation for the observed emission is synchrotron radiation formed by shocked host media via interactions between active galactic nucleus winds and the host environment.…”
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112
Hot Accretion Flow in Two-Dimensional Spherical Coordinates: Considering Pressure Anisotropy and Magnetic Field
Published 2019-09-01“…Outflows from an active galactic nucleus can interact with gas in its host galaxies. …”
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113
Investigating Ionization in the Intergalactic Medium
Published 2024-01-01“…Energetic processes, such as galactic feedback from star formation and active galactic nucleus winds, would be excellent candidates that can cause such widespread ionization.…”
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114
Observing—and Imaging—Active Galactic Nuclei with the Event Horizon Telescope
Published 2018“…Originally developed to image the shadow region of the central black hole in Sagittarius A* and in the nearby galaxy M87, the Event Horizon Telescope (EHT) provides deep, very high angular resolution data on other active galactic nucleus (AGN) sources too. The challenges of working with EHT data have spurred the development of new image reconstruction algorithms. …”
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115
Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube
Published 2022“…These dusty objects are generally powered by starbursts with star formation rates that exceed 100 M⊙ yr−1, possibly combined with a contribution from an active galactic nucleus. Such environments make ULIRGs plausible sources of astrophysical high-energy neutrinos, which can be observed by the IceCube Neutrino Observatory at the South Pole. …”
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116
Vigorous star formation in a bulge-dominated extremely red object at z=1.34
Published 2005“…There is no evidence that the galaxy contains an active galactic nucleus. Analysis of a further two targets, which do not exhibit any features in our near-IR spectra, suggests that one is a quiescent galaxy in the redshift range 1.2 < z < 1.6, but that the other cannot be conclusively categorized as either star-forming or quiescent. …”
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117
High-redshift obscured quasars: radio emission at sub-kiloparsec scales
Published 2009“…The physical extent of this emission is ~<150 pc, and the derived properties indicate that this emission originates from an active galactic nucleus (AGN). The missing flux density is difficult to account for by star-formation alone, so radio components associated with jets of physical size >~150 pc, and ~< 40 kpc are likely to be present in most of the sources. …”
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118
Herschel observations and a model for IRAS 08572+3915: a candidate for the most luminous infrared galaxy in the local (z < 0.2) Universe
Published 2014“…The model suggests that this object is powered by an active galactic nucleus (AGN) with a fairly smooth torus viewed almost edge-on and a very young starburst. …”
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119
Obscured activity: AGN, quasars, starbursts and ULIGs observed by the infrared space observatory
Published 2005“…ISO surveyed a wide range of active galaxies which, in the context of this review, includes those powered by intense bursts of star formation as well as those containing a dominant active galactic nucleus (AGN). Mid-infrared imaging resolved for the first time the dust enshrouded nuclei in many nearby galaxies, while a new era in infrared spectroscopy was opened by probing a wealth of atomic, ionic and molecular lines as well as broad band features in the mid- and far-infrared. …”
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120
Galaxy Zoo: The properties of merging galaxies in the nearby Universe - Local environments, colours, masses, star formation rates and AGN activity
Published 2010“…Following the study of Darg et al., we explore the environments, optical colours, stellar masses, star formation and active galactic nucleus activity in a sample of 3003 pairs of merging galaxies drawn from the Sloan Digital Sky Survey using visual classifications from the Galaxy Zoo project. …”
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