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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.authorVučetić, M. M.en_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
dc.relation.ispartofAstrophysical Journalen
dc.subjectISM: magnetic fieldsen
dc.subjectISM: supernova remnantsen
dc.subjectradio continuum: generalen
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.urlhttps://api.elsevier.com/content/abstract/scopus_id/84886890726-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.volume777en
dc.relation.issue1en
item.fulltextNo Fulltext-
item.openairetypeArticle-
item.grantfulltextnone-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.cerifentitytypePublications-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-8036-4132-
crisitem.author.orcid0000-0003-0665-0939-
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