Detailed abundance study of four s-process enriched post-AGB stars in the Large Magellanic Cloud

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dc.contributor.authorvan Aarle, Els
dc.contributor.authorvan Winckel, Hans
dc.contributor.authorDe Smedt, K
dc.contributor.authorKamath, Devika
dc.contributor.authorWood, Peter R
dc.date.accessioned2015-12-13T22:24:57Z
dc.date.issued2013
dc.date.updated2016-02-24T09:12:54Z
dc.description.abstractContext. The photospheric abundances of evolved solar-type stars of different metallicities serve as probes into stellar evolution theory. Aims. Stellar photospheres of post-asymptotic giant branch (post-AGB) stars bear witness to the internal chemical en
dc.identifier.issn0004-6361
dc.identifier.urihttp://hdl.handle.net/1885/73006
dc.publisherSpringer
dc.rightsAuthor/s retain copyrighten_AU
dc.sourceAstronomy and Astrophysics
dc.subjectKeywords: Circumstellar matters; Magellanic Clouds; Stars: abundances; Stars: evolution; Stars:AGB and post AGB; Astrophysics; Chemical elements; Galaxies; Mercury (metal); Neutron irradiation; Stars Circumstellar matter; Magellanic Clouds; Stars: abundances; Stars: AGB and post-AGB; Stars: evolution
dc.titleDetailed abundance study of four s-process enriched post-AGB stars in the Large Magellanic Cloud
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.lastpage14)
local.bibliographicCitation.startpageA106 (1
local.contributor.affiliationvan Aarle, Els, Instituut voor Sterrenkunde
local.contributor.affiliationvan Winckel, Hans, Instituut voor Sterrenkunde
local.contributor.affiliationDe Smedt, K, Instituut voor Sterrenkunde
local.contributor.affiliationKamath, Devika, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationWood, Peter R, College of Physical and Mathematical Sciences, ANU
local.contributor.authoruidKamath, Devika, u4602544
local.contributor.authoruidWood, Peter R, u7900259
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationf5625xPUB3520
local.identifier.citationvolume554
local.identifier.doi10.1051/0004-6361/201219988
local.identifier.scopusID2-s2.0-84878974208
local.identifier.thomsonID000320444200105
local.type.statusPublished Version

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