Please use this identifier to cite or link to this item:
https://research.matf.bg.ac.rs/handle/123456789/810| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Arbutina, Bojan | en_US |
| dc.date.accessioned | 2022-08-15T16:03:20Z | - |
| dc.date.available | 2022-08-15T16:03:20Z | - |
| dc.date.issued | 2015-04-29 | - |
| dc.identifier.issn | 19903413 | en |
| dc.identifier.uri | https://research.matf.bg.ac.rs/handle/123456789/810 | - |
| dc.description.abstract | Blast 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 |
| dc.relation.ispartof | Astrophysical Bulletin | en |
| dc.subject | general | en |
| dc.subject | shock waves—supernovae | en |
| dc.title | Blast waves with cosmic rays | en_US |
| dc.type | Article | en_US |
| dc.identifier.doi | 10.1134/S1990341315020078 | - |
| dc.identifier.scopus | 2-s2.0-84930206098 | - |
| dc.identifier.url | https://api.elsevier.com/content/abstract/scopus_id/84930206098 | - |
| dc.contributor.affiliation | Astronomy | en_US |
| dc.relation.firstpage | 214 | en |
| dc.relation.lastpage | 219 | en |
| dc.relation.volume | 70 | en |
| dc.relation.issue | 2 | en |
| item.fulltext | No Fulltext | - |
| item.openairetype | Article | - |
| item.grantfulltext | none | - |
| item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
| item.cerifentitytype | Publications | - |
| crisitem.author.dept | Astronomy | - |
| crisitem.author.orcid | 0000-0002-8036-4132 | - |
| Appears in Collections: | Research outputs | |
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