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.
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Broad Iron Lines in Active Galactic Nuclei
TL;DR: In this article, the authors summarize the physics of the fluorescent line formation and show that Fe Kα line profile observations can be used to probe relativistic effects in the vicinity of the black hole, concentrating on recent results from XMM-Newton.
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A full characterization of the supermassive black hole in IRAS 09149–6206
Dom Walton,William Alston,P. Kosec,A. C. Fabian,Luigi C. Gallo,Javier A. García,Jon M. Miller,E. Nardini,E. Nardini,Mark Reynolds,Claudio Ricci,Claudio Ricci,Claudio Ricci,D. Stern,Thomas Dauser,Fiona A. Harrison,Christopher S. Reynolds +16 more
TL;DR: In this paper, the authors present new broadband X-ray observations of the type-I Seyfert galaxy IRAS 09149-6206, taken in 2018 with $XMM$-$Newton$, $NuSTAR$ and $Swift$.
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Efficient Production of Sound Waves by AGN Jets in the Intracluster Medium
TL;DR: In this article, the authors investigated the efficiency with which jets can drive sound waves into the ICM and found that high velocity, wide angle jets produce sound waves most efficiently, yet the acoustic efficiency never exceeds 1/3 of the jet energy.
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Global Simulations of Accretion Disks I: Convergence and Comparisons with Local Models
TL;DR: In this paper, a set of global grid-based magnetohydrodynamic (MHD) simulations was performed for the study of astrophysical accretion disks, and the authors showed that the saturation of the MHD turbulence via parasitic modes of the magnetorotational instability is related to the instantaneous correlations between local flux and stress found in global simulations.
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An ionized accretion disc wind in Hercules X-1
TL;DR: In this article, an ionized wind was detected in the high-energy X-ray spectrum of Herculis X-1 when the source is in the very high state.