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Gamma-Ray Flares from the Crab Nebula

Gamma-Ray Flares from the Crab Nebula

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_swepub_primary_oai_DiVA_org_su_67516

Gamma-Ray Flares from the Crab Nebula

About this item

Full title

Gamma-Ray Flares from the Crab Nebula

Publisher

Washington, DC: American Association for the Advancement of Science

Journal title

Science (American Association for the Advancement of Science), 2011-02, Vol.331 (6018), p.739-742

Language

English

Formats

Publication information

Publisher

Washington, DC: American Association for the Advancement of Science

More information

Scope and Contents

Contents

A young and energetic pulsar powers the well-known Crab Nebula. Here, we describe two separate gamma-ray (photon energy greater than 100 mega-electron volts) flares from this source detected by the Large Area Telescope on board the Fermi Gamma-ray Space Telescope. The first flare occurred in February 2009 and lasted approximately 16 days. The secon...

Alternative Titles

Full title

Gamma-Ray Flares from the Crab Nebula

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_swepub_primary_oai_DiVA_org_su_67516

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_swepub_primary_oai_DiVA_org_su_67516

Other Identifiers

ISSN

0036-8075,1095-9203

E-ISSN

1095-9203

DOI

10.1126/science.1199705