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Optical superluminal motion measurement in the neutron-star merger GW170817

Optical superluminal motion measurement in the neutron-star merger GW170817

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_2724584265

Optical superluminal motion measurement in the neutron-star merger GW170817

About this item

Full title

Optical superluminal motion measurement in the neutron-star merger GW170817

Publisher

London: Nature Publishing Group UK

Journal title

Nature (London), 2022-10, Vol.610 (7931), p.273-276

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

The afterglow of the binary neutron-star merger GW170817
1
gave evidence for a structured relativistic jet
2

6
and a link
3
,
7
,
8
between such mergers and short gamma-ray bursts. Superluminal motion, found using radio very long baseline interferometry
3
(VLBI), together with the afterglow light curve pr...

Alternative Titles

Full title

Optical superluminal motion measurement in the neutron-star merger GW170817

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_miscellaneous_2724584265

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_2724584265

Other Identifiers

ISSN

0028-0836

E-ISSN

1476-4687

DOI

10.1038/s41586-022-05145-7

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