Stephen P. Reynolds
Stephen P. Reynolds from North Carolina State University, was awarded the status of Fellow in the American Physical Society, after he was nominated by his Division of Astrophysics in 2000, for ''contributions to high-energy astrophysics, including modeling relativistic jets in quasars, pulsar-driven supernova remnants, and electron acceleration to synchrotron X-ray emitting energies in young shell supernova remnants, and supporting observations.'' Provided by Wikipedia
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An X-Ray Synchrotron Shell and a Pulsar: The Peculiar Supernova Remnant G32.4+0.1 by Stephen P. Reynolds, Kazimierz J. Borkowski
Published 2024-01-01
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A Broadband X-Ray Study of the Rabbit Pulsar Wind Nebula Powered by PSR J1418-6058 by Jaegeun Park, Chanho Kim, Jooyun Woo, Hongjun An, Kaya Mori, Stephen P. Reynolds, Samar Safi-Harb
Published 2023-01-01
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X-Ray Characterization of the Pulsar PSR J1849−0001 and Its Wind Nebula G32.64+0.53 Associated with TeV Sources Detected by H.E.S.S., HAWC, Tibet ASγ, and LHAASO by Chanho Kim, Jaegeun Park, Jooyun Woo, Sarah Silverman, Hongjun An, Aya Bamba, Kaya Mori, Stephen P. Reynolds, Samar Safi-Harb
Published 2023-01-01
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Rapid Expansion of the Young Type Ia Supernova Remnant 0519–69.0: More Evidence for a Circumstellar Shell by Benson T. Guest, Kazimierz J. Borkowski, Parviz Ghavamian, Robert Petre, Adrien Picquenot, Stephen P. Reynolds, Ivo R. Seitenzahl, Brian J. Williams
Published 2023-01-01
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