Please use this identifier to cite or link to this item: https://open.uns.ac.rs/handle/123456789/713
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dc.contributor.authorProdanović, Tijanaen_US
dc.contributor.authorĆiprijanović, Aleksandraen_US
dc.date.accessioned2019-09-23T10:10:26Z-
dc.date.available2019-09-23T10:10:26Z-
dc.date.issued2019-01-01-
dc.identifier.isbn9783030138752en_US
dc.identifier.issn09308989en_US
dc.identifier.urihttps://open.uns.ac.rs/handle/123456789/713-
dc.description.abstract© 2019, Springer Nature Switzerland AG. It has been shown that galactic interactions and mergers can result in large-scale tidal shocks that propagate through interstellar gas. As a result, this can give rise to a new population of cosmic rays, additional to standard galactic cosmic rays present in star-forming galaxies. We investigate the impact of this tidal cosmic-ray population on the nucleosynthesis of light elements. We especially focus on extragalactic systems where lithium has been measured in gas phase but which have been disturbed by galactic interactions, namely the Small Magellanic Cloud and the M82. Moreover, we demonstrate that the presence of these tidal shock-waves may also have far reaching consequences on star-formation rate estimates and our general understanding of galactic evolution through affecting the far-infrared radio correlation.en
dc.relation.ispartofSpringer Proceedings in Physicsen
dc.titleCosmic-Ray Nucleosynthesis in Galactic Interactionsen_US
dc.typeConference Paperen_US
dc.identifier.doi10.1007/978-3-030-13876-9_79-
dc.identifier.scopus2-s2.0-85071907208-
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/85071907208-
dc.description.versionUnknownen_US
dc.relation.lastpage420en
dc.relation.firstpage417en
dc.relation.volume219en
item.fulltextNo Fulltext-
item.grantfulltextnone-
crisitem.author.deptPrirodno-matematički fakultet, Departman za fiziku-
crisitem.author.parentorgPrirodno-matematički fakultet-
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