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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/258
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dc.contributor.authorOnić, D.en_US
dc.contributor.authorUrošević, Dejanen_US
dc.date.accessioned2022-08-06T17:48:09Z-
dc.date.available2022-08-06T17:48:09Z-
dc.date.issued2015-06-01-
dc.identifier.issn0004637Xen
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/258-
dc.description.abstractThe integrated radio spectrum of Cassiopeia A in continuum was analyzed with special emphasis on possible high-frequency spectral curvature. We conclude that the most probable scenario is that Planck's new data reveal the imprint of nonlinear particle acceleration in the case of this young Galactic supernova remnant.en
dc.relation.ispartofAstrophysical Journalen
dc.subjectacceleration of particlesen
dc.subjectISM: individual objects (Cas A)en
dc.subjectISM: supernova remnantsen
dc.subjectradiation mechanisms: non-thermalen
dc.subjectradio continuum: ISMen
dc.titleOn the continuum radio spectrum of CAS A: Possible evidence of nonlinear particle accelerationen_US
dc.typeArticleen_US
dc.identifier.doi10.1088/0004-637X/805/2/119-
dc.identifier.scopus2-s2.0-84934878828-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84934878828-
dc.contributor.affiliationAstronomyen_US
dc.relation.volume805en
dc.relation.issue2en
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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