The X-ray counterpart to the gravitational-wave event GW170817-Reference-Cited by-同舟云学术

The X-ray counterpart to the gravitational-wave event GW170817

Published:2017-10-16 Issue:7678 Volume:551 Page:71-74
ISSN:0028-0836
Container-title:Nature
language:en
Short-container-title:Nature

Author:

Troja E.,Piro L.,van Eerten H.,Wollaeger R. T.,Im M.,Fox O. D.,Butler N. R.,Cenko S. B.,Sakamoto T.,Fryer C. L.,Ricci R.,Lien A.,Ryan R. E.,Korobkin O.,Lee S.-K.,Burgess J. M.,Lee W. H.,Watson A. M.,Choi C.,Covino S.,D’Avanzo P.,Fontes C. J.,González J. Becerra,Khandrika H. G.,Kim J.,Kim S.-L.,Lee C.-U.,Lee H. M.,Kutyrev A.,Lim G.,Sánchez-Ramírez R.,Veilleux S.,Wieringa M. H.,Yoon Y.

Publisher

Springer Science and Business Media LLC

Subject

Multidisciplinary

Link

http://www.nature.com/articles/nature24290.pdf

Reference81 articles.

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3. Rezzolla, L. et al. The missing link: merging neutron stars naturally produce jet-like structures and can power short gamma-ray bursts. Astrophys. J. 732, L6 (2011)

4. Gehrels, N. et al. A short γ-ray burst apparently associated with an elliptical galaxy at redshift z = 0.225. Nature 437, 851–854 (2005)

5. Berger, E. Short-duration gamma-ray bursts. Annu. Rev. Astron. Astrophys. 52, 43–105 (2014)

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