Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/250
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dc.contributor.authorArbutina, Bojanen_US
dc.contributor.authorUrošević, Dejanen_US
dc.contributor.authorAnđelić, Milicaen_US
dc.contributor.authorPavlović, M. Z.en_US
dc.contributor.authorVukotić, B.en_US
dc.date.accessioned2022-08-06T17:48:08Z-
dc.date.available2022-08-06T17:48:08Z-
dc.date.issued2013-11-01-
dc.identifier.issn0004637Xen
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/250-
dc.description.abstractThe equipartition or minimum energy calculation is a well-known procedure for estimating the magnetic field strength and the total energy in the magnetic field and cosmic ray particles by using only the radio synchrotron emission. In one of our previous papers, we have offered a modified equipartition calculation for supernova remnants (SNRs) with spectral indices 0.5 < α < 1. Here we extend the analysis to SNRs with α = 0.5 and α = 1. © 2013. The American Astronomical Society. All rights reserved.en_US
dc.language.isoenen_US
dc.publisherIOP Scienceen_US
dc.relation.ispartofAstrophysical Journalen_US
dc.subjectISM: magnetic fieldsen_US
dc.subjectISM: supernova remnantsen_US
dc.subjectradio continuum: generalen_US
dc.titleModified equipartition calculation for supernova remnants. Cases α = 0.5 and α = 1en_US
dc.typeArticleen_US
dc.identifier.doi10.1088/0004-637X/777/1/31-
dc.identifier.scopus2-s2.0-84886890726-
dc.identifier.isi000326147300031-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84886890726-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.issn0004-637Xen_US
dc.description.rankM21aen_US
dc.relation.firstpageArticle no. 31en_US
dc.relation.volume777en_US
dc.relation.issue1en_US
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairetypeArticle-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextNo Fulltext-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-8036-4132-
crisitem.author.orcid0000-0003-0665-0939-
crisitem.author.orcid0000-0003-3146-234X-
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