Electromagnetic evidence that SSS17a is the result of a binary neutron star merger

被引:222
作者
Kilpatrick, C. D. [1 ]
Foley, R. J. [1 ]
Kasen, D. [2 ,3 ,4 ]
Murguia-Berthier, A. [1 ]
Ramirez-Ruiz, E. [1 ,5 ]
Coulter, D. A. [1 ]
Drout, M. R. [6 ]
Piro, A. L. [6 ]
Shappee, B. J. [6 ,7 ]
Boutsia, K. [8 ]
Contreras, C. [8 ]
Di Mille, F. [8 ]
Madore, B. F. [6 ]
Morrell, N. [8 ]
Pan, Y-C. [1 ]
Prochaska, J. X. [1 ]
Rest, A. [9 ,10 ]
Rojas-Bravo, C. [1 ]
Siebert, M. R. [1 ]
Simon, J. D. [6 ]
Ulloa, N. [11 ]
机构
[1] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA
[2] Lawrence Berkeley Natl Lab, Div Nucl Sci, Berkeley, CA 94720 USA
[3] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA
[4] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[5] Univ Copenhagen, Niels Bohr Inst, DARK, Blegdamsvej 17, DK-2100 Copenhagen, Denmark
[6] Observ Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 USA
[7] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA
[8] Carnegie Observ, Las Campanas Observ, Casilla 601, La Serena, Chile
[9] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA
[10] Johns Hopkins Univ, Dept Phys & Astron, 3400 North Charles St, Baltimore, MD 21218 USA
[11] Univ La Serena, Fac Ciencias, Dept Fis & Astron, Cisternas 1200, La Serena, Chile
基金
新加坡国家研究基金会; 美国国家科学基金会; 美国国家航空航天局;
关键词
PROGENITORS; ELEMENTS; SUPERNOVAE; MASS;
D O I
10.1126/science.aaq0073
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
Eleven hours after the detection of gravitational wave source GW170817 by the Laser Interferometer Gravitational-Wave Observatory and Virgo Interferometers, an associated optical transient, SSS17a, was identified in the galaxy NGC 4993. Although the gravitational wave data indicate that GW170817 is consistent with the merger of two compact objects, the electromagnetic observations provide independent constraints on the nature of that system. We synthesize the optical to near-infrared photometry and spectroscopy of SSS17a collected by the One-Meter Two-Hemisphere collaboration, finding that SSS17a is unlike other known transients. The source is best described by theoretical models of a kilonova consisting of radioactive elements produced by rapid neutron capture (the r-process). We conclude that SSS17a was the result of a binary neutron star merger, reinforcing the gravitational wave result.
引用
收藏
页码:1583 / 1587
页数:5
相关论文
共 39 条
[1]   Characterization of the LIGO detectors during their sixth science run [J].
Aasi, J. ;
Abadie, J. ;
Abbott, B. P. ;
Abbott, R. ;
Abbott, T. ;
Abernathy, M. R. ;
Accadia, T. ;
Acernese, F. ;
Adams, C. ;
Adams, T. ;
Adhikari, R. X. ;
Affeldt, C. ;
Agathos, M. ;
Aggarwal, N. ;
Aguiar, O. D. ;
Ajith, P. ;
Allen, B. ;
Allocca, A. ;
Ceron, E. Amador ;
Amariutei, D. ;
Anderson, R. A. ;
Anderson, S. B. ;
Anderson, W. G. ;
Arai, K. ;
Araya, M. C. ;
Arceneaux, C. ;
Areeda, J. ;
Ast, S. ;
Aston, S. M. ;
Astone, P. ;
Aufmuth, P. ;
Aulbert, C. ;
Austin, L. ;
Aylott, B. E. ;
Babak, S. ;
Baker, P. T. ;
Ballardin, G. ;
Ballmer, S. W. ;
Barayoga, J. C. ;
Barker, D. ;
Barnum, S. H. ;
Barone, F. ;
Barr, B. ;
Barsotti, L. ;
Barsuglia, M. ;
Barton, M. A. ;
Bartos, I. ;
Bassiri, R. ;
Basti, A. ;
Batch, J. .
CLASSICAL AND QUANTUM GRAVITY, 2015, 32 (11)
[2]  
Abbott BP, 2017, PHYS REV LETT, V118, DOI [10.1103/PhysRevLett.118.221101, 10.1103/PhysRevLett.118.121102]
[3]   UPPER LIMITS ON THE RATES OF BINARY NEUTRON STAR AND NEUTRON STAR-BLACK HOLE MERGERS FROM ADVANCED LIGO'S FIRST OBSERVING RUN [J].
Abbott, B. P. ;
Abbott, R. ;
Abbott, T. D. ;
Abernathy, M. R. ;
Acernese, E. ;
Ackley, K. ;
Adams, C. ;
Adams, T. ;
Addesso, P. ;
Adhikari, R. X. ;
Adya, V. B. ;
Affeldt, C. ;
Agathos, M. ;
Agatsuma, K. ;
Aggarwal, N. ;
Aguiar, O. D. ;
Aiello, L. ;
Ain, A. ;
Ajith, P. ;
Allen, B. ;
Allocca, A. ;
Altin, P. A. ;
Anderson, S. B. ;
Anderson, W. G. ;
Arai, K. ;
Araya, M. C. ;
Arceneaux, C. C. ;
Areeda, J. S. ;
Arnaud, N. ;
Arun, K. G. ;
Ascenzi, S. ;
Ashton, G. ;
Ast, M. ;
Aston, S. M. ;
Astone, P. ;
Aufmuth, P. ;
Aulbert, C. ;
Babak, S. ;
Bacon, P. ;
Bader, M. K. M. ;
Baker, P. T. ;
Baldaccini, F. ;
Ballardin, G. ;
Ballmer, S. W. ;
Barayoga, J. C. ;
Barclay, S. E. ;
Barish, B. C. ;
Barker, D. ;
Barone, E. ;
Barr, B. .
ASTROPHYSICAL JOURNAL LETTERS, 2016, 832 (02)
[4]   Advanced Virgo: a second-generation interferometric gravitational wave detector [J].
Acernese, F. ;
Agathos, M. ;
Agatsuma, K. ;
Aisa, D. ;
Allemandou, N. ;
Allocca, A. ;
Amarni, J. ;
Astone, P. ;
Balestri, G. ;
Ballardin, G. ;
Barone, F. ;
Baronick, J-P ;
Barsuglia, M. ;
Basti, A. ;
Basti, F. ;
Bauer, Th S. ;
Bavigadda, V. ;
Bejger, M. ;
Beker, M. G. ;
Belczynski, C. ;
Bersanetti, D. ;
Bertolini, A. ;
Bitossi, M. ;
Bizouard, M. A. ;
Bloemen, S. ;
Blom, M. ;
Boer, M. ;
Bogaert, G. ;
Bondi, D. ;
Bondu, F. ;
Bonelli, L. ;
Bonnand, R. ;
Boschi, V. ;
Bosi, L. ;
Bouedo, T. ;
Bradaschia, C. ;
Branchesi, M. ;
Briant, T. ;
Brillet, A. ;
Brisson, V. ;
Bulik, T. ;
Bulten, H. J. ;
Buskulic, D. ;
Buy, C. ;
Cagnoli, G. ;
Calloni, E. ;
Campeggi, C. ;
Canuel, B. ;
Carbognani, F. ;
Cavalier, F. .
CLASSICAL AND QUANTUM GRAVITY, 2015, 32 (02)
[5]  
[Anonymous], ARXIV170807885ASTROP
[6]   EFFECT OF A HIGH OPACITY ON THE LIGHT CURVES OF RADIOACTIVELY POWERED TRANSIENTS FROM COMPACT OBJECT MERGERS [J].
Barnes, Jennifer ;
Kasen, Daniel .
ASTROPHYSICAL JOURNAL, 2013, 775 (01)
[7]   SYSTEMATICS OF DYNAMICAL MASS EJECTION, NUCLEOSYNTHESIS, AND RADIOACTIVELY POWERED ELECTROMAGNETIC SIGNALS FROM NEUTRON-STAR MERGERS [J].
Bauswein, A. ;
Goriely, S. ;
Janka, H. -T. .
ASTROPHYSICAL JOURNAL, 2013, 773 (01)
[8]   Faint thermonuclear supernovae from AM Canum Venaticorum binaries [J].
Bildsten, Lars ;
Shen, Ken J. ;
Weinberg, Nevin N. ;
Nelemans, Gijs .
ASTROPHYSICAL JOURNAL, 2007, 662 (02) :L95-L98
[9]   IN SEARCH OF THE PROGENITORS OF TYPE IA SUPERNOVAE [J].
BRANCH, D ;
LIVIO, M ;
YUNGELSON, LR ;
BOFFI, FR ;
BARON, E .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 1995, 107 (717) :1019-1029
[10]   SYNTHESIS OF THE ELEMENTS IN STARS [J].
BURBIDGE, EM ;
BURBIDGE, GR ;
FOWLER, WA ;
HOYLE, F .
REVIEWS OF MODERN PHYSICS, 1957, 29 (04) :547-650