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HIGH-ENERGY TRANSIENTS

HIGH-ENERGY TRANSIENTS

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_pascalfrancis_primary_4957499

HIGH-ENERGY TRANSIENTS

About this item

Full title

HIGH-ENERGY TRANSIENTS

Author / Creator

Publisher

Legacy CDMS: The Astronomical Society of the Pacific

Journal title

Publications of the Astronomical Society of the Pacific, 1991-08, Vol.103 (666), p.760-769

Language

English

Formats

Publication information

Publisher

Legacy CDMS: The Astronomical Society of the Pacific

More information

Scope and Contents

Contents

X-ray and y-ray bursts are high-energy transients that usually last ~ 1-100 seconds but otherwise have quite different properties. X-ray bursts are thought to come from weakly magnetic neutron stars, while new observational and theoretical work provides powerful evidence that many y-ray bursts come from strongly magnetic neutron stars. In this revi...

Alternative Titles

Full title

HIGH-ENERGY TRANSIENTS

Authors, Artists and Contributors

Author / Creator

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_pascalfrancis_primary_4957499

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_pascalfrancis_primary_4957499

Other Identifiers

ISSN

0004-6280

E-ISSN

1538-3873

DOI

10.1086/132876

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