Submitted by Astro-ph Robot on Wed, 10/15/2014 - 00:47
"An Ultraluminous X-ray Source Powered by An Accreting Neutron Star."M. Bachetti,
F. A. Harrison,
D. J. Walton,
B. W. Grefenstette,
D. Chakrabarty,
F. Fürst,
D. Barret,
A. Beloborodov,
S. E. Boggs,
F. E. Christensen,
W. W. Craig,
A. C. Fabian,
C. J. Hailey,
A. Hornschemeier,
V. Kaspi,
S.R. Kulkarni,
T. Maccarone,
J. M. Miller,
V. Rana,
D. Stern,
S. P. Tendulkar,
J. Tomsick,
N. A. Webb,
W. W. Zhang.
"A new look at the cosmic ray positron fraction."M. Boudaud,
S. Aupetit,
S. Caroff,
A. Putze,
G. Belanger,
Y. Genolini,
C. Goy,
V. Poireau,
V. Poulin,
S. Rosier,
P. Salati,
L. Tao,
M. Vecchi.
