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

Mihoko Yukita, Andrew Ptak, Thomas Maccarone, Ann E Hornschemeier, Daniel R Wik, Katja Pottschmidt, Valsamo Antoniou, Frederick K Baganoff, Bret Lehmer, Andreas Zezas

Research output: Contribution to conferencePaper

Original languageEnglish
StatePublished - 2016

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    Yukita, M., Ptak, A., Maccarone, T., Hornschemeier, A. E., Wik, D. R., Pottschmidt, K., Antoniou, V., Baganoff, F. K., Lehmer, B., & Zezas, A. (2016). 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.