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The X-ray counterpart to the gravitational wave event GW 170817

The X-ray counterpart to the gravitational wave event GW 170817

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2076319658

The X-ray counterpart to the gravitational wave event GW 170817

About this item

Full title

The X-ray counterpart to the gravitational wave event GW 170817

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2017-10

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

A long-standing paradigm in astrophysics is that collisions- or mergers- of two neutron stars (NSs) form highly relativistic and collimated outflows (jets) powering gamma-ray bursts (GRBs) of short (< 2 s) duration. However, the observational support for this model is only indirect. A hitherto outstanding prediction is that gravitational wave (GW)...

Alternative Titles

Full title

The X-ray counterpart to the gravitational wave event GW 170817

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2076319658

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2076319658

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.1710.05433

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