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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/810
DC FieldValueLanguage
dc.contributor.authorArbutina, Bojanen_US
dc.date.accessioned2022-08-15T16:03:20Z-
dc.date.available2022-08-15T16:03:20Z-
dc.date.issued2015-04-29-
dc.identifier.issn19903413en
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/810-
dc.description.abstractBlast waves appear in many astrophysical phenomena, such as supernovae. In this paper we discuss blast waves with cosmic rays, i.e., with a component with a power-law number density distribution function N(p) ∝ p<sup>−Γ</sup> that may be particulary important in describing the evolution of supernova remnants. We confirm some previous findings that a significant amount of cosmic ray energy is deposited towards the center of a remnant.en_US
dc.language.isoenen_US
dc.publisherSpringeren_US
dc.relation.ispartofAstrophysical Bulletinen_US
dc.subjectgeneralen_US
dc.subjectshock waves—supernovaeen_US
dc.titleBlast waves with cosmic raysen_US
dc.typeArticleen_US
dc.identifier.doi10.1134/S1990341315020078-
dc.identifier.scopus2-s2.0-84930206098-
dc.identifier.isi000355210300007-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/84930206098-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn1990-3413en_US
dc.description.rankM22en_US
dc.relation.firstpage214en_US
dc.relation.lastpage219en_US
dc.relation.volume70en_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.orcid0000-0002-8036-4132-
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