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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/255
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dc.contributor.authorBozzetto, L. M.en_US
dc.contributor.authorFilipović, M. D.en_US
dc.contributor.authorUrošević, Dejanen_US
dc.contributor.authorCrawford, E. J.en_US
dc.date.accessioned2022-08-06T17:48:09Z-
dc.date.available2022-08-06T17:48:09Z-
dc.date.issued2012-12-01-
dc.identifier.issn1450698Xen
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/255-
dc.description.abstractWe report on new Australian Telescope Compact Array (ATCA) observations of SNR J0519-6902. The Supernova Remnant (SNR) is small in size (~8 pc) and exhibits a typical SNR spectrum with α = -0.53 ± 0.07, with steeper spectral indices towards the northern limb of the remnant. SNR J0519-6902 con-tains a low level of radially orientated polarisation at wavelengths of 3 and 6 cm, which is typical of younger SNRs. A fairly strong magnetic field was estimated to ~171 μG. The remnant appears to be the result of a typical Type Ia super-nova, sharing many properties with another small and young Type Ia LMC SNR, J0509-6731.en
dc.relation.ispartofSerbian Astronomical Journalen
dc.subjectIndividual objectsen
dc.subjectIsmen
dc.subjectIsm-ismen
dc.subjectMagellanic cloudsen
dc.subjectRadio continuumen
dc.subjectSnr j0519-6902en
dc.subjectSupernova remnantsen
dc.titleRadio-continuum observations of small, radially polarised supernova remnant j0519-6902 in the large magellanic clouden_US
dc.typeArticleen_US
dc.identifier.doi10.2298/SAJ1285025B-
dc.identifier.scopus2-s2.0-84872194976-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84872194976-
dc.contributor.affiliationAstronomyen_US
dc.relation.firstpage25en
dc.relation.lastpage33en
dc.relation.issue185en
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0003-0665-0939-
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