Three-dimensional simulations of the expanding remnant of SN 1987A

dc.contributor.authorPotter, Tobyen
dc.contributor.authorStaveley-Smith, Listeren
dc.contributor.authorKirk, Johnen
dc.contributor.authorReville, Brianen
dc.contributor.authorBicknell, Geoffen
dc.contributor.authorSutherland, Ralphen
dc.contributor.authorWagner, Alexanderen
dc.contributor.authorZanardo, Giovannaen
dc.date.accessioned2025-06-10T22:39:29Z
dc.date.available2025-06-10T22:39:29Z
dc.date.issued2014en
dc.description.abstractSNR 1987A is the expanding remnant from the brightest supernova since the invention of the telescope. The remnant has been monitored extensively in the radio at variety of wavelengths and provides a wealth of data on which to base a simulation. Questions to be answered include estimating the efficiency of particle acceleration at shock fronts, determining the cause of the one-sided radio morphology for SNR 1987A and investigating the gas properties of the pre-supernova environment. We attempt to address these questions using a fully three-dimensional model of SNR 1987A.en
dc.description.statusPeer-revieweden
dc.format.extent2en
dc.identifier.isbn9781107044777en
dc.identifier.issn1743-9213en
dc.identifier.scopus84897868625en
dc.identifier.urihttp://www.scopus.com/inward/record.url?scp=84897868625&partnerID=8YFLogxKen
dc.identifier.urihttps://hdl.handle.net/1885/733757966
dc.language.isoenen
dc.relation.ispartofSupernova Environmental Impactsen
dc.relation.ispartofseriesProceedings of the International Astronomical Unionen
dc.relation.isversionofS296en
dc.subjectparticle accelerationen
dc.subjectsimulationen
dc.subjectSN 1987Aen
dc.subjectSupernovaeen
dc.subjectthree-dimensionalen
dc.titleThree-dimensional simulations of the expanding remnant of SN 1987Aen
dc.typeConference paperen
dspace.entity.typePublicationen
local.bibliographicCitation.lastpage331en
local.bibliographicCitation.startpage330en
local.contributor.affiliationPotter, Toby; University of Western Australiaen
local.contributor.affiliationStaveley-Smith, Lister; University of Western Australiaen
local.contributor.affiliationKirk, John; Max Planck Institute for Nuclear Physicsen
local.contributor.affiliationReville, Brian; University of Oxforden
local.contributor.affiliationBicknell, Geoff; RSAA - Stromlo, Research School of Astronomy & Astrophysics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationSutherland, Ralph; RSAA - Stromlo, Research School of Astronomy & Astrophysics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationWagner, Alexander; RSAA - Stromlo, Research School of Astronomy & Astrophysics, ANU College of Science and Medicine, The Australian National Universityen
local.contributor.affiliationZanardo, Giovanna; University of Western Australiaen
local.identifier.ariespublicationU3488905xPUB2628en
local.identifier.doi10.1017/S1743921313009678en
local.identifier.essn1743-9221en
local.identifier.pure58aee0cd-3a46-4b45-a07a-8e5ec21bb3a8en
local.identifier.urlhttps://www.scopus.com/pages/publications/84897868625en
local.type.statusPublisheden

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