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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/3099
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dc.contributor.authorAlsaberi, Rami Z.E.en_US
dc.contributor.authorFilipović, Miroslav D.en_US
dc.contributor.authorSano, Hidetoshien_US
dc.contributor.authorDai, Shien_US
dc.contributor.authorHaberl, Franken_US
dc.contributor.authorKavanagh, Patrick J.en_US
dc.contributor.authorLeahy, Denisen_US
dc.contributor.authorMaggi, Pierreen_US
dc.contributor.authorRowell, Gavinen_US
dc.contributor.authorSasaki, Manamien_US
dc.contributor.authorSeitenzahl, Ivo R.en_US
dc.contributor.authorUrošević, Dejanen_US
dc.contributor.authorPayne, Jeffreyen_US
dc.contributor.authorSmeaton, Zachary J.en_US
dc.contributor.authorLazarević, Sanjaen_US
dc.date.accessioned2026-01-17T12:05:15Z-
dc.date.available2026-01-17T12:05:15Z-
dc.date.issued2025-06-04-
dc.identifier.issn13233580-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/3099-
dc.description.abstractWe present a new radio continuum study of the Large Magellanic Cloud supernova remnant (SNR) MC SNR J0519-6902. With a diameter of 8 pc, this SNR shows a radio ring-like morphology with three bright regions towards the north, east, and south. Its linear polarisation is prominent with average values of % and % at 5500 and 9000 MHz, and we find a spectral index of, typical of a young SNR. The average rotation measure is estimated at rad m and the magnetic field strength at G. We also estimate an equipartition magnetic field of G and minimum explosion energy of E = 2.6 erg. Finally, we identified an H i cloud that may be associated with MC SNR J0519-6902, located in the southeastern part of the remnant, along with a potential wind-bubble cavity.en_US
dc.language.isoenen_US
dc.publisherCambridge : Cambridge University Pressen_US
dc.relation.ispartofPublications of the Astronomical Society of Australiaen_US
dc.subjectgalaxies: Magellanic Cloudsen_US
dc.subjectISM: supernova remnantsen_US
dc.subjectmethods: observationalen_US
dc.titleA new radio continuum study of the large magellanic cloud supernova remnant MC SNR J0519-6902en_US
dc.typeArticleen_US
dc.identifier.doi10.1017/pasa.2025.10025-
dc.identifier.scopus2-s2.0-105007667169-
dc.identifier.isi001520472600001-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/105007667169-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1323-3580en_US
dc.description.rankM21aen_US
dc.relation.firstpageArticle no. e069en_US
dc.relation.volume42en_US
item.openairetypeArticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextnone-
item.fulltextNo Fulltext-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0003-0665-0939-
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