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Please use this identifier to cite or link to this item: https://research.matf.bg.ac.rs/handle/123456789/260
DC FieldValueLanguage
dc.contributor.authorUrošević, Dejanen_US
dc.date.accessioned2022-08-06T17:48:09Z-
dc.date.available2022-08-06T17:48:09Z-
dc.date.issued2020-10-01-
dc.identifier.urihttps://research.matf.bg.ac.rs/handle/123456789/260-
dc.description.abstractThe determination of the evolutionary stage for a supernova remnant is a demanding task. This guide for radio observers presents a relatively straightforward way to establish the evolutionary phase of newly observed supernova remnants.en_US
dc.language.isoenen_US
dc.publisherSpringer Natureen_US
dc.relation.ispartofNature Astronomyen_US
dc.subjectinterstellar mediumen_US
dc.subjectstellar evolutionen_US
dc.titleDetermining the evolutionary status of supernova remnantsen_US
dc.typeArticleen_US
dc.identifier.doi10.1038/s41550-020-01228-5-
dc.identifier.scopus2-s2.0-85091348972-
dc.identifier.isi000572294500001-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85091348972-
dc.contributor.affiliationAstronomyen_US
dc.relation.issn2397-3366en_US
dc.description.rankM21aen_US
dc.relation.firstpage910en_US
dc.relation.lastpage912en_US
dc.relation.volume4en_US
dc.relation.issue10en_US
item.openairetypeArticle-
item.cerifentitytypePublications-
item.fulltextNo Fulltext-
item.grantfulltextnone-
item.languageiso639-1en-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
crisitem.author.deptAstronomy-
crisitem.author.orcid0000-0003-0665-0939-
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