Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6404
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dc.contributor.authorCui, W. Y-
dc.contributor.authorSivarani, T-
dc.contributor.authorChristlieb, N-
dc.date.accessioned2013-10-10T14:08:50Z-
dc.date.available2013-10-10T14:08:50Z-
dc.date.issued2013-10-
dc.identifier.citationAstronomy and Astrophysics, Vol. 558, A36en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/6404-
dc.descriptionOpen Accessen
dc.description.abstractAims. The aim of this study is a detailed abundance analysis of the newly discovered r-rich star HE 1405−0822, which has [Fe/H] = −2.40. This star shows enhancements of both r- and s-elements, [Ba/Fe] = + 1.95 and [Eu/Fe] = 1.54, for which reason it is called r+s star. Methods. Stellar parameters and element abundances were determined by analyzing high-quality VLT/UVES spectra. We used Fe I line excitation equilibria to derive the effective temperature. The surface gravity was calculated from the Fe i/Fe ii and Ti i/Ti ii equilibria. Results. We determined accurate abundances for 39 elements, including 19 neutron-capture elements. HE 1405−0822 is a red giant. Its strong enhancements of C, N, and s-elements are the consequence of enrichment by a former AGB companion with an initial mass of less than 3 M⊙. The heavy n-capture element abundances (including Eu, Yb, and Hf) seen in HE 1405−0822 do not agree with the r-process pattern seen in strongly r-process-enhanced stars. We discuss possible enrichment scenarios for this star. The enhanced α elements can be explained as the result of enrichment by supernovae of type II. Na and Mg may have partly been synthesized in a former AGB companion, when the primary 22Ne acted as a neutron poison in the 13C-pocketen
dc.language.isoenen
dc.publisherEDP Sciencesen
dc.relation.urihttp://dx.doi.org/10.1051/0004-6361/201321597en
dc.relation.urihttp://arxiv.org/abs/1308.4492en
dc.rights© ESOen
dc.subjectStars: abundancesen
dc.subjectStars: AGB and post-AGBen
dc.subjectStars: atmospheresen
dc.subjectStars: chemically peculiaren
dc.titleThe Hamburg/ESO R-process Enhanced Star survey (HERES) VIII. The r+s star HE 1405 0822en
dc.typeArticleen
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