C
Christopher S. Reynolds
Researcher at University of Cambridge
Publications - 570
Citations - 37823
Christopher S. Reynolds is an academic researcher from University of Cambridge. The author has contributed to research in topics: Active galactic nucleus & Galaxy. The author has an hindex of 95, co-authored 541 publications receiving 34690 citations. Previous affiliations of Christopher S. Reynolds include University of Maryland, College Park & Tohoku Gakuin University.
Papers
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Suzaku Observations of Local Ultraluminous Infrared Galaxies
Stacy H. Teng,Sylvain Veilleux,Naohisa Anabuki,Charles D. Dermer,Luigi C. Gallo,Takao Nakagawa,Christopher S. Reynolds,David B. Sanders,Yuichi Terashima,Andrew S. Wilson +9 more
TL;DR: In this paper, the absorption-corrected log[$L 2-10 keV/$ / $L_{\rm IR}$] ratio is consistent with those found in PG Quasars.
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Accretion disk dynamo as the trigger for X-ray binary state transitions
TL;DR: In this paper, a simple model for the creation of a toroidal magnetic field and its coupling to the gas was proposed, and it was shown how disks could be driven into this magnetically dominated state and deduced the resulting vertical pressure and density profiles.
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2MASX J00423991+3017515: An offset active galactic nucleus in an interacting system.
J. Drew Hogg,J. Drew Hogg,Laura Blecha,Christopher S. Reynolds,Krista Lynne Smith,Lisa M. Winter +5 more
TL;DR: In this article, the authors presented a spectroscopic and imaging study of an abnormal active galactic nucleus (AGN), 2MASX J00423991+3017515, which was newly identified in the hard X-rays by the Swift BAT All-Sky survey and found in an edge-on disk galaxy interacting with a nearby companion.
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The Disk-Wind-Jet Connection in the Black Hole H 1743-322
Jon M. Miller,John C. Raymond,Andrew C. Fabian,Christopher S. Reynolds,Ashley L. King,Timothy R. Kallman,Edward M. Cackett,M. van der Klis,Danny Steeghs +8 more
TL;DR: In this paper, the authors present an analysis of a deep, 60 ksec Chandra/HETGS observation of the black hole candidate H 1743-322 in the low/hard state, with tight limits, and within the range of ionizing flux levels that were measured in prior Chandra observations wherein a wind was clearly detected.
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Nustar view of the central region of the Perseus cluster
TL;DR: NuSTAR observations of 3C 84 have been reported in this article, showing that the power-law component dominates the spectrum above 20 keV with a photon index of ∼1.9 and an energy flux of 1.0.