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Viewing Angle of Binary Neutron Star Mergers

Viewing Angle of Binary Neutron Star Mergers

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_78aa5dc0cb3f46bba95c73c7746f1601

Viewing Angle of Binary Neutron Star Mergers

About this item

Full title

Viewing Angle of Binary Neutron Star Mergers

Publisher

College Park: American Physical Society

Journal title

Physical review. X, 2019-08, Vol.9 (3), p.031028, Article 031028

Language

English

Formats

Publication information

Publisher

College Park: American Physical Society

More information

Scope and Contents

Contents

The joint detection of the gravitational wave (GW) GW170817 and its electromagnetic (EM) counterparts GRB170817A and kilonova AT 2017gfo has triggered extensive study of the EM emission of binary neutron star mergers. A parameter which is common to and plays a key role in both the GW and the EM analyses is the viewing angle of the binary’s orbit. I...

Alternative Titles

Full title

Viewing Angle of Binary Neutron Star Mergers

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_doaj_primary_oai_doaj_org_article_78aa5dc0cb3f46bba95c73c7746f1601

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_doaj_primary_oai_doaj_org_article_78aa5dc0cb3f46bba95c73c7746f1601

Other Identifiers

ISSN

2160-3308

E-ISSN

2160-3308

DOI

10.1103/PhysRevX.9.031028

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