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Stephen P. Reynolds

Researcher at North Carolina State University

Publications -  243
Citations -  14382

Stephen P. Reynolds is an academic researcher from North Carolina State University. The author has contributed to research in topics: Supernova & Supernova remnant. The author has an hindex of 58, co-authored 232 publications receiving 13302 citations. Previous affiliations of Stephen P. Reynolds include University of North Carolina at Chapel Hill & Harvard University.

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THE NUCLEAR SPECTROSCOPIC TELESCOPE ARRAY (NuSTAR) HIGH-ENERGY X-RAY MISSION

Fiona A. Harrison, +84 more
TL;DR: The Nuclear Spectroscopic Telescope Array (NuSTAR) as discussed by the authors is the first focusing high-energy X-ray telescope in orbit, which operates in the band from 3 to 79 keV.
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The Nuclear Spectroscopic Telescope Array (NuSTAR) Mission

TL;DR: The Nuclear Spectroscopic Telescope Array (NuSTAR) as discussed by the authors is the first focusing high-energy X-ray telescope in orbit, which operates in the band from 3 - 79 keV.
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Supernova Remnants in the Sedov Expansion Phase: Thermal X-Ray Emission

TL;DR: In this article, a new set of Sedov models for supernova remnants (SNRs) in the Sedov-Taylor phase is reported, which allows for a partial collisionless heating of electrons at the blast wave and for energy transfer from ions to electrons through Coulomb collisions.
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Supernova Remnants at High Energy

TL;DR: In this paper, a review examines the relevant characteristics of Type Ia and core-collapse supernovae, the dynamics of their evolution through the Sedov blast-wave phase, the basic physics of diffusive shock acceleration, and the physics of relevant radiative processes.
Journal ArticleDOI

Supernova Remnants in the Sedov Expansion Phase: Thermal X-Ray Emission

TL;DR: In this article, improved calculations of X-ray spectra for supernova remnants (SNRs) in the Sedov-Taylor phase are reported, which for the first time include reliable atomic data for Fe L-shell lines.