Submitted by Astro-ph Robot on Tue, 03/21/2017 - 20:47
"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.