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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/258
DC FieldValueLanguage
dc.contributor.authorOnić, Dušanen_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_US
dc.language.isoenen_US
dc.publisherIOP Scienceen_US
dc.relation.ispartofAstrophysical Journalen_US
dc.subjectacceleration of particlesen_US
dc.subjectISM: individual objects (Cas A)en_US
dc.subjectISM: supernova remnantsen_US
dc.subjectradiation mechanisms: non-thermalen_US
dc.subjectradio continuum: ISMen_US
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.isi000356715400034-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84934878828-
dc.contributor.affiliationAstronomyen_US
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1538-4357en_US
dc.description.rankM21aen_US
dc.relation.firstpageArticle no. 119en_US
dc.relation.volume805en_US
dc.relation.issue2en_US
item.openairetypeArticle-
item.fulltextNo Fulltext-
item.languageiso639-1en-
item.cerifentitytypePublications-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.grantfulltextnone-
crisitem.author.deptAstronomy-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0002-2130-2011-
crisitem.author.orcid0000-0003-0665-0939-
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