X-Ray Measurements of the Particle Acceleration Properties at Inward Shocks in Cassiopeia A
We present new evidence that the bright nonthermal X-ray emission features in the interior of the Cassiopeia A supernova remnant are caused by inward-moving shocks, based on Chandra and NuSTAR observations. Several bright inward-moving filaments were identified using monitoring data taken by Chandra...
Main Authors: | Sato, Toshiki, Katsuda, Satoru, Morii, Mikio, Bamba, Aya, Hughes, John P., Maeda, Yoshitomo, Ishida, Manabu, Fraschetti, Federico |
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Other Authors: | Univ Arizona, Dept Planetary Sci & Astron |
Language: | en |
Published: |
IOP PUBLISHING LTD
2018
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Subjects: | |
Online Access: | http://hdl.handle.net/10150/626534 http://arizona.openrepository.com/arizona/handle/10150/626534 |
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