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Detection of Gamma-Ray Emission from the Vela Pulsar Wind Nebula with AGILE

Detection of Gamma-Ray Emission from the Vela Pulsar Wind Nebula with AGILE

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_swepub_primary_oai_DiVA_org_kth_85818

Publication information

Publisher

United States: American Association for the Advancement of Science

More information

Scope and Contents

Contents

Pulsars are known to power winds of relativistic particles that can produce bright nebulae by interacting with the surrounding medium. These pulsar wind nebulae are observed by their radio, optical, and x-ray emissions, and in some cases also at TeV (teraelectron volt) energies, but the lack of information in the gamma-ray band precludes drawing a...

Alternative Titles

Full title

Detection of Gamma-Ray Emission from the Vela Pulsar Wind Nebula with AGILE

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_swepub_primary_oai_DiVA_org_kth_85818

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_swepub_primary_oai_DiVA_org_kth_85818

Other Identifiers

ISSN

0036-8075,1095-9203

E-ISSN

1095-9203

DOI

10.1126/science.1183844

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