Accession Number:

AD1105707

Title:

Multi-Messenger Observations of a Binary Neutron Star Merger

Descriptive Note:

Journal Article - Open Access

Corporate Author:

NAVAL RESEARCH LAB WASHINGTON DC WASHINGTON United States

Report Date:

2017-10-16

Pagination or Media Count:

59.0

Abstract:

n 2017 August 17 a binary neutron star coalescence candidate later designated GW170817 with merger time124104 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. TheFermi Gamma-ray Burst Monitor independently detected a gamma-ray burst GRB 170817A with a time delay of1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a skyregion of 31 deg2 at a luminosity distance of 40 88- Mpc and with component masses consistent with neutron stars. Thecomponent masses were later measured to be in the range 0.86 to 2.26 M. An extensive observing campaign waslaunched across the electromagnetic spectrum leading to the discovery of a bright optical transient SSS17a, now withthe IAU identification of AT 2017gfo in NGC 4993 at 40 Mpc less than 11 hours after the merger by the One-Meter, Two Hemisphere 1M2H team using the 1 m Swope Telescope. The optical transient was independentlydetected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Earlyultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed aredward evolution over 10 days. Following early non-detections, X-ray and radio emission were discovered atthe transients position 9 and 16 days, respectively, after the merger. Both the X-ray and radio emission likelyarise from a physical process that is distinct from the one that generates the UVopticalnear-infrared emission. Noultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches.These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst GRB 170817A and a kilonovamacronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta.

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Distribution Statement:

APPROVED FOR PUBLIC RELEASE