Submitted by Astro-ph Robot on Wed, 03/22/2017 - 00:47
"Identification of the Hard X-ray Source Dominating the E > 25 keV Emission of the Nearby Galaxy M31."M. Yukita,
A. Ptak,
A. E. Hornschemeier,
D. Wik,
T. J. Maccarone,
K. Pottschmidt,
A. Zezas,
V. Antoniou,
R. Ballhausen,
B. D. Lehmer,
A. Lien,
B. Williams,
F. Baganoff,
P. T. Boyd,
T. Enoto,
J. Kennea,
K. L. Page,
Y. Choi.
