NuSTAR STUDY OF HARD X-RAY MORPHOLOGY AND SPECTROSCOPY OF PWN G21.5–0.9

We present NuSTAR high-energy X-ray observations of the pulsar wind nebula (PWN)/supernova remnant G21.5–0.9. We detect integrated emission from the nebula up to ~40 keV, and resolve individual spatial features over a broad X-ray band for the first time. The morphology seen by NuSTAR agrees well wit...

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Автори: Nynka, Melania, Hailey, Charles J., Reynolds, Stephen P., An, Hongjun, Boggs, Steven E., Christensen, Finn E., Craig, William W., Gotthelf, Eric V., Grefenstette, Brian W., Harrison, Fiona A., Krivonos, Roman A., Madsen, Kristin K., Mori, Kaya, Perez, Kerstin, Stern, Daniel, Wik, Daniel R., Zhang, William W., Zoglauer, Andreas, Baganoff, Frederick K
Інші автори: MIT Kavli Institute for Astrophysics and Space Research
Формат: Стаття
Мова:en_US
Опубліковано: IOP Publishing 2015
Онлайн доступ:http://hdl.handle.net/1721.1/92935