What dominates the X-ray emission of Andromeda at E&gt;20 keV? New constraints from NuSTAR and Swift on a very bright, hard X-ray source

What dominates the X-ray emission of Andromeda at E>20 keV? New constraints from NuSTAR and Swift on a very bright, hard X-ray source

Published in 2016 by Mihoko Yukita, Andrew Ptak, Thomas J. Maccarone, Ann E. Hornschemeier, Daniel R. Wik, Katja Pottschmidt, Vallia Antoniou, Frederick K. Baganoff, Bret Lehmer, Andreas Zezas, Patricia T. Boyd, Jamie Kennea, Kim L. Page

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