A kilonova as the electromagnetic counterpart to a gravitational-wave source

被引：0
|
作者：
S. J. Smartt
T.-W. Chen
A. Jerkstrand
M. Coughlin
E. Kankare
S. A. Sim
M. Fraser
C. Inserra
K. Maguire
K. C. Chambers
M. E. Huber
T. Krühler
G. Leloudas
M. Magee
L. J. Shingles
K. W. Smith
D. R. Young
J. Tonry
R. Kotak
A. Gal-Yam
J. D. Lyman
D. S. Homan
C. Agliozzo
J. P. Anderson
C. R. Angus
C. Ashall
C. Barbarino
F. E. Bauer
M. Berton
M. T. Botticella
M. Bulla
J. Bulger
G. Cannizzaro
Z. Cano
R. Cartier
A. Cikota
P. Clark
A. De Cia
M. Della Valle
L. Denneau
M. Dennefeld
L. Dessart
G. Dimitriadis
N. Elias-Rosa
R. E. Firth
H. Flewelling
A. Flörs
A. Franckowiak
C. Frohmaier
L. Galbany
机构：
[1] Astrophysics Research Centre,Department of Physics and Astronomy
[2] School of Mathematics and Physics,Department of Particle Physics and Astrophysics
[3] Queens University Belfast,Department of Physics
[4] Max-Planck-Institut für Extraterrestrische Physik,Departamento de Ciencias Fisicas
[5] Max-Planck Institut für Astrophysik,Department of Astronomy
[6] LIGO Laboratory West Bridge,Dipartimento di Fisica e Astronomia ‘G. Galilei’
[7] Room 257 California Institute of Technology,Department of Physics
[8] School of Physics,Department of Astrophysics/IMAPP
[9] O’Brien Centre for Science North,Departamento de Astronomía
[10] University College Dublin,Physik
[11] University of Southampton,Department
[12] Institute for Astronomy,Department of Physics and Astronomy
[13] University of Hawaii,Department of Physics and Astronomy
[14] Dark Cosmology Centre,Department of Physics
[15] Niels Bohr Institute,Department of Astrophysics
[16] University of Copenhagen,Department of Astronomy
[17] Weizmann Institute of Science,Department of Physics and Astronomy
[18] University of Warwick,Department of Physics
[19] Institute for Astronomy,Department of Physics
[20] SUPA (Scottish Universities Physics Alliance),Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA) and Department of Physics and Astronomy
[21] University of Edinburgh,undefined
[22] Royal Observatory,undefined
[23] Universidad Andres Bello,undefined
[24] Millennium Institute of Astrophysics (MAS),undefined
[25] European Southern Observatory,undefined
[26] Astrophysics Research Institute,undefined
[27] Liverpool John Moores University,undefined
[28] IC2,undefined
[29] The Oskar Klein Centre,undefined
[30] Stockholm University,undefined
[31] Instituto de Astrofísica and Centro de Astroingeniería,undefined
[32] Facultad de Física,undefined
[33] Pontificia Universidad Católica de Chile,undefined
[34] Space Science Institute,undefined
[35] Università di Padova,undefined
[36] INAF — Osservatorio Astronomico di Brera,undefined
[37] INAF — Osservatorio Astronomico di Capodimonte,undefined
[38] The Oskar Klein Centre,undefined
[39] Stockholm University,undefined
[40] SRON,undefined
[41] Netherlands Institute for Space Research,undefined
[42] Radboud University,undefined
[43] Instituto de Astrofísica de Andalucía (IAA-CSIC),undefined
[44] Glorieta de la Astronomía,undefined
[45] European Southern Observatory,undefined
[46] ICRANet-Pescara,undefined
[47] IAP/CNRS and University Pierre et Marie Curie,undefined
[48] Unidad Mixta Internacional Franco-Chilena de Astronomía (CNRS UMI 3386),undefined
[49] Universidad de Chile,undefined
[50] Istituto Nazionale di Astrofisica,undefined
来源：
Nature | 2017年 / 551卷
关键词：
D O I：
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中图分类号：
学科分类号：
摘要：
Observations and modelling of an optical transient counterpart to a gravitational-wave event and γ-ray burst reveal that neutron-star mergers produce gravitational waves and radioactively powered kilonovae, and are a source of heavy elements.
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页码：75 / 79
页数：4
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