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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2156
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dc.contributor.authorKameswara Rao, N-
dc.contributor.authorReddy, B. E-
dc.date.accessioned2008-03-14T10:50:56Z-
dc.date.available2008-03-14T10:50:56Z-
dc.date.issued2005-02-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 357, No. 1, pp. 235 – 241en
dc.identifier.urihttp://hdl.handle.net/2248/2156-
dc.descriptionRestricted Accessen
dc.description.abstractAnalysis of the surface composition of the suspected cool RV Tauri star CE Virginis shows no systematic trend in depletions of elements with respect to condensation temperature. However, there is a significant depletion of the elements with respect to the first ionization potential of the element. The derived Li abundance of log ε (Li) = 1.5 ± 0.2 indicates production of Li in the star. Near-infrared colours indicate sporadic dust formation close to the photosphere.en
dc.format.extent227679 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherBlackwell Publishingen
dc.relation.urihttp://www.blackwell-synergy.com/doi/abs/10.1111/j.1365-2966.2005.08636.xen
dc.relation.urihttp://arxiv.org/abs/astro-ph/0411481en
dc.subjectstars: abundancesen
dc.subjectstars: individual: CE Virginisen
dc.subjectstars: individual: RV Taurien
dc.subjectstars: individual: SRd variablesen
dc.titleHigh-resolution spectroscopy of the high galactic latitude RV Tauri star CE Virginisen
dc.typeArticleen
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