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...
Автори: | , , , , , , , , , , , , , , , , , , |
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Інші автори: | |
Формат: | Стаття |
Мова: | en_US |
Опубліковано: |
IOP Publishing
2015
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Онлайн доступ: | http://hdl.handle.net/1721.1/92935 |