Submitted by Astro-ph Robot on Sun, 06/16/2019 - 20:47
"Discovery of a 2.8 s pulsar in a 2 d orbit High-Mass X-ray Binary powering the Ultraluminous X-ray source ULX-7 in M51."G. A. Rodríguez Castillo,
G. L. Israel,
A. Belfiore,
F. Bernardini,
P. Esposito,
F. Pintore,
A. De Luca,
A. Papitto,
L. Stella,
A. Tiengo,
L. Zampieri,
M. Bachetti,
M. Brightman,
P. Casella,
D. D'Agostino,
S. Dall'Osso,
H. P. Earnshaw,
F. Füst,
F. Haberl,
F. A. Harrison,
M. Mapelli,
M. Marelli,
M. Middleton,
C. Pinto,
T. P. Roberts,
R. Salvaterra,
R. Turolla,
D. J. Walton,
A. Wolter.
"Constraining the Neutron Star Compactness: Extraction of the $^{23}$Al($p,\gamma$) Reaction Rate for the $rp$-Process."C. Wolf,
C. Langer,
F. Montes,
J. Pereira,
W.-J. Ong,
T. Poxon-Pearson,
S. Ahn,
S. Ayoub,
T. Baumann,
D. Bazin,
P.C. Bender,
B.A. Brown,
J. Browne,
H. Crawford,
R.H. Cyburt,
E. Deleeuw,
B. Elman,
S. Fiebiger,
A. Gade,
P. Gastis,
S. Lipschutz,
B. Longfellow,
Z. Meisel,
F.M. Nunes,
G. Perdikakis,
R. Reifarth,
W.A. Richter,
H. Schatz,
K. Schmidt,
J. Schmitt,
C. Sullivan,
R. Titus,
D. Weisshaar,
P.J. Woods,
J.C. Zamora,
R.G.T. Zegers.
