The Binary Neutron Star Event LIGO/Virgo GW170817 160 Days after Merger: Synchrotron Emission across the Electromagnetic Spectrum-Reference-Cited by-同舟云学术

The Binary Neutron Star Event LIGO/Virgo GW170817 160 Days after Merger: Synchrotron Emission across the Electromagnetic Spectrum

Published:2018-03-23 Issue:1 Volume:856 Page:L18
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Margutti R.^ORCID,Alexander K. D.^ORCID,Xie X.,Sironi L.,Metzger B. D.^ORCID,Kathirgamaraju A.,Fong W.^ORCID,Blanchard P. K.,Berger E.^ORCID,MacFadyen A.^ORCID,Giannios D.,Guidorzi C.^ORCID,Hajela A.,Chornock R.,Cowperthwaite P. S.,Eftekhari T.,Nicholl M.^ORCID,Villar V. A.,Williams P. K. G.,Zrake J.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/aab2ad/pdf

Reference90 articles.

1. GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2. Particle acceleration by ultrarelativistic shocks: theory and simulations

3. The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. VI. Radio Constraints on a Relativistic Jet and Predictions for Late-time Emission from the Kilonova Ejecta

4. Relativistic outflows from remnants of compact object mergers and their viability for short gamma-ray bursts

5. The acceleration of cosmic rays in shock fronts - I

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