A Strong Jet Signature in the Late-time Light Curve of GW170817-Reference-Cited by-同舟云学术

A Strong Jet Signature in the Late-time Light Curve of GW170817

Published:2018-11-16 Issue:1 Volume:868 Page:L11
ISSN:2041-8213
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Mooley K. P.^ORCID,Frail D. A.,Dobie D.^ORCID,Lenc E.^ORCID,Corsi A.^ORCID,De K.,Nayana A. J.,Makhathini S.,Heywood I.,Murphy T.^ORCID,Kaplan D. L.^ORCID,Chandra P.,Smirnov O.,Nakar E.,Hallinan G.^ORCID,Camilo F.^ORCID,Fender R.,Goedhart S.,Groot P.,Kasliwal M. M.^ORCID,Kulkarni S. R.^ORCID,Woudt P. A.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/2041-8213/aaeda7/pdf

Reference81 articles.

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

2. Multi-messenger Observations of a Binary Neutron Star Merger

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. A Decline in the X-Ray through Radio Emission from GW170817 Continues to Support an Off-axis Structured Jet

5. Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger

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