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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/62868
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dc.contributor.authorClay, R.-
dc.contributor.authorWhelan, B.-
dc.contributor.authorEdwards, P.-
dc.date.issued2010-
dc.identifier.citationPublications of the Astronomical Society of Australia, 2010; 27(4):439-448-
dc.identifier.issn1323-3580-
dc.identifier.issn1448-6083-
dc.identifier.urihttp://hdl.handle.net/2440/62868-
dc.descriptionSubmitted to Cornell University’s online archive www.arXiv.org in 2010 by Benjamin Whelan. Post-print sourced from www.arxiv.org-
dc.description.abstract<jats:title>Abstract</jats:title><jats:p>We review the importance of Centaurus A in high-energy astrophysics as a nearby object with many of the properties expected of a major source of very high-energy cosmic rays and gamma rays. We examine observational techniques and the results so far obtained in the energy range from 200 GeV to above 100 EeV and attempt to fit those data to expectations of Centaurus Aas an astrophysical source from very high to ultra-high energies.</jats:p>-
dc.language.isoen-
dc.publisherC S I R O Publishing-
dc.rightsCopyright © 2010 Astronomical Society of Australia-
dc.source.urihttp://arxiv.org/abs/1001.0813-
dc.titleCentaurus A at ultra-high energies-
dc.typeJournal article-
dc.identifier.doi10.1071/AS09077-
pubs.publication-statusPublished-
dc.identifier.orcidClay, R. [0000-0002-9040-9648]-
Appears in Collections:Aurora harvest 5
IPAS publications
Physics publications

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