LOCATING THE MOST ENERGETIC ELECTRONS IN CASSIOPEIA A

LOCATING THE MOST ENERGETIC ELECTRONS IN CASSIOPEIA A

We present deep (>2.4 Ms) observations of the Cassiopeia A supernova remnant with NuSTAR, which operates in the 3–79 keV bandpass and is the first instrument capable of spatially resolving the remnant above 15 keV. We find that the emission is not entirely dominated by the forward shock nor by a...

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Bibliographic Details
Main Authors: Grefenstette, Brian W., Reynolds, Stephen P., Harrison, Fiona A., Humensky, T. Brian, Boggs, Steven E., Fryer, Chris L., DeLaney, Tracey, Madsen, Kristin K., Miyasaka, Hiromasa, Wik, Daniel R., Zoglauer, Andreas, Forster, Karl, Kitaguchi, Takao, Nynka, Melania, Christensen, Finn E., Craig, William W., Hailey, Charles J., Stern, Daniel, Zhang, William W., Lopez, Laura A.
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:en_US
Published: IOP Publishing 2015
Online Access:http://hdl.handle.net/1721.1/97082

Internet

http://hdl.handle.net/1721.1/97082

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