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A very-high-energy component deep in the γ-ray burst afterglow

A very-high-energy component deep in the γ-ray burst afterglow

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_swepub_primary_oai_DiVA_org_lnu_90546

A very-high-energy component deep in the γ-ray burst afterglow

About this item

Full title

A very-high-energy component deep in the γ-ray burst afterglow

Publisher

London: Nature Publishing Group UK

Journal title

Nature (London), 2019-11, Vol.575 (7783), p.464-467

Language

English

Formats

Publication information

Publisher

London: Nature Publishing Group UK

More information

Scope and Contents

Contents

Gamma-ray bursts (GRBs) are brief flashes of γ-rays and are considered to be the most energetic explosive phenomena in the Universe
1
. The emission from GRBs comprises a short (typically tens of seconds) and bright prompt emission, followed by a much longer afterglow phase. During the afterglow phase, the shocked outflow—produced by the inte...

Alternative Titles

Full title

A very-high-energy component deep in the γ-ray burst afterglow

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_swepub_primary_oai_DiVA_org_lnu_90546

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_swepub_primary_oai_DiVA_org_lnu_90546

Other Identifiers

ISSN

0028-0836,1476-4687

E-ISSN

1476-4687

DOI

10.1038/s41586-019-1743-9