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Barium and iron abundances in red giants

dc.contributor.authorFernández Villacañas, J. L.
dc.contributor.authorRego Fernández, Manuel
dc.contributor.authorCornide Castro-Piñeiro, Manuel
dc.date.accessioned2023-06-20T20:08:43Z
dc.date.available2023-06-20T20:08:43Z
dc.date.issued1990-06
dc.description© 1990 American Astronomical Society. © 1990 IOP Publishing.
dc.description.abstractAn intermediate-dispersion abundance analysis has been carried out on a sample of 21 barium and 14 comparison stars. The excess of barium over iron has been used as the most representative indicator of peculiarity. These excesses are higher in the peculiar stars than in the nonpeculiar stars. Particularly interesting is the case of HD 67447, included in the comparison stars, with an excess Ba/Fe abundance = 1.61, probably a new barium star. A trend indicating a possible anticorrelation between barium overabundance and metallicity favors the suggestion that the "barium strong" group is older than the "barium weak" one.
dc.description.departmentDepto. de Física de la Tierra y Astrofísica
dc.description.facultyFac. de Ciencias Físicas
dc.description.refereedTRUE
dc.description.statuspub
dc.eprint.idhttps://eprints.ucm.es/id/eprint/31390
dc.identifier.doi10.1086/115478
dc.identifier.issn0004-6256
dc.identifier.officialurlhttp://dx.doi.org/10.1086/115478
dc.identifier.relatedurlhttp://adsabs.harvard.edu/
dc.identifier.relatedurlhttp://iopscience.iop.org
dc.identifier.urihttps://hdl.handle.net/20.500.14352/59668
dc.issue.number6
dc.journal.titleAstronomical journal
dc.language.isoeng
dc.page.final1970
dc.page.initial1961
dc.publisherIOP Publishing ltd
dc.rights.accessRightsopen access
dc.subject.cdu52
dc.subject.keywordAstronomy
dc.subject.keywordAstrophysics
dc.subject.ucmAstrofísica
dc.subject.ucmAstronomía (Física)
dc.titleBarium and iron abundances in red giants
dc.typejournal article
dc.volume.number99
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