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Properties of the binary neutron star merger GW170817

Properties of the binary neutron star merger GW170817

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2073341664

Properties of the binary neutron star merger GW170817

About this item

Full title

Properties of the binary neutron star merger GW170817

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2019-01

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

On August 17, 2017, the Advanced LIGO and Advanced Virgo gravitational-wave detectors observed a low-mass compact binary inspiral. The initial sky localization of the source of the gravitational-wave signal, GW170817, allowed electromagnetic observatories to identify NGC 4993 as the host galaxy. In this work, we improve initial estimates of the bin...

Alternative Titles

Full title

Properties of the binary neutron star merger GW170817

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2073341664

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2073341664

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.1805.11579

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