Evidence for X-Ray Emission in Excess to the Jet-afterglow Decay 3.5 yr after the Binary Neutron Star Merger GW 170817: A New Emission Component

Authors :: A. Hajela
R. Margutti
J. S. Bright
K. D. Alexander
B. D. Metzger
V. Nedora
A. Kathirgamaraju
B. Margalit
D. Radice
C. Guidorzi
E. Berger
A. MacFadyen
D. Giannios
R. Chornock
I. Heywood
L. Sironi
O. Gottlieb
D. Coppejans
T. Laskar
Y. Cendes
R. Barniol Duran
T. Eftekhari
W. Fong
A. McDowell
M. Nicholl
X. Xie
J. Zrake
S. Bernuzzi
F. S. Broekgaarden
C. D. Kilpatrick
G. Terreran
V. A. Villar
P. K. Blanchard
S. Gomez
G. Hosseinzadeh
D. J. Matthews
J. C. Rastinejad
Source :: The Astrophysical Journal Letters. 927(1):L17
Publication Year :: 2022
Publisher :: United States: NASA Center for Aerospace Information (CASI), 2022.

Language :: English
ISSN :: 20418213 and 20418205
Volume :: 927
Issue :: 1
Database :: NASA Technical Reports
Journal :: The Astrophysical Journal Letters
Notes :: AST-1909796, , AST-1944985, , G09-20058A, , #15606, , #80NSSC19K1422
Publication Type :: Report
Accession number :: edsnas.22678847628185
Document Type :: Report
Full Text :: https://doi.org/10.3847/2041-8213/ac504a

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