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Swift and NuSTAR observations of GW170817: Detection of a blue kilonova

Evans, PA; Cenko, SB; Kennea, JA; Emery, SWK; Kuin, NPM; Korobkin, O; Wollaeger, RT; ... Tohuvavohu, A; + view all (2017) Swift and NuSTAR observations of GW170817: Detection of a blue kilonova. Science 10.1126/science.aap9580. Green open access

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Abstract

With the first direct detection of merging black holes in 2015, the era of gravitational wave (GW) astrophysics began. A complete picture of compact object mergers, however, requires the detection of an electromagnetic (EM) counterpart. We report ultraviolet (UV) and x-ray observations by Swift and the Nuclear Spectroscopic Telescope ARray (NuSTAR) of the EM counterpart of the binary neutron star merger GW 170817. The bright, rapidly fading ultraviolet emission indicates a high mass (≈ 0.03 solar masses) wind-driven outflow with moderate electron fraction (Ye ≈ 0.27). Combined with the x-ray limits, we favor an observer viewing angle of ≈30° away from the orbital rotation axis, which avoids both obscuration from the heaviest elements in the orbital plane and a direct view of any ultra-relativistic, highly collimated ejecta (a γ-ray burst afterglow).

Type: Article
Title: Swift and NuSTAR observations of GW170817: Detection of a blue kilonova
Location: United States
Open access status: An open access version is available from UCL Discovery
DOI: 10.1126/science.aap9580
Publisher version: http://dx.doi.org/10.1126/science.aap9580
Language: English
Additional information: This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10025009
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