Please use this identifier to cite or link to this item: https://open.uns.ac.rs/handle/123456789/13782
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dc.contributor.authorBikit I.en
dc.contributor.authorLakosi L.en
dc.contributor.authorSáfár J.en
dc.contributor.authorČonkić L.en
dc.date.accessioned2020-03-03T14:53:41Z-
dc.date.available2020-03-03T14:53:41Z-
dc.date.issued1999-09-01en
dc.identifier.issn0004637Xen
dc.identifier.urihttps://open.uns.ac.rs/handle/123456789/13782-
dc.description.abstractThe 180mTa (γ, γ′) 180Ta reaction was induced by gamma rays from a strong 60Co source. Population of the ground state was observed (effective cross section 0.12 ± 0.02 μbarns) with an integrated cross section of 0.13 ± 0.04 μbarns MeV through mediating levels assumed near 1 MeV. Transition multi-polarities and astrophysical consequences are discussed.en
dc.relation.ispartofAstrophysical Journalen
dc.titleDe-excitation of <sup>180m</sup>Ta by <sup>60</sup>Co gamma raysen
dc.typeJournal/Magazine Articleen
dc.identifier.scopus2-s2.0-0033193779en
dc.identifier.urlhttps://api.elsevier.com/content/abstract/scopus_id/0033193779en
dc.relation.lastpage423en
dc.relation.firstpage419en
dc.relation.issue1 PART 1en
dc.relation.volume522en
item.grantfulltextnone-
item.fulltextNo Fulltext-
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