High-resolution spectroscopy of the high galactic latitude RV Tauri star CE Virginis

dc.contributor.author	Kameswara Rao, N
dc.contributor.author	Reddy, B. E
dc.date.accessioned	2008-03-14T10:50:56Z
dc.date.available	2008-03-14T10:50:56Z
dc.date.issued	2005-02
dc.identifier.citation	Monthly Notices of the Royal Astronomical Society, Vol. 357, No. 1, pp. 235 – 241	en
dc.identifier.uri	http://hdl.handle.net/2248/2156
dc.description	Restricted Access	en
dc.description.abstract	Analysis 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.extent	227679 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Blackwell Publishing	en
dc.relation.uri	http://www.blackwell-synergy.com/doi/abs/10.1111/j.1365-2966.2005.08636.x	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/0411481	en
dc.subject	stars: abundances	en
dc.subject	stars: individual: CE Virginis	en
dc.subject	stars: individual: RV Tauri	en
dc.subject	stars: individual: SRd variables	en
dc.title	High-resolution spectroscopy of the high galactic latitude RV Tauri star CE Virginis	en
dc.type	Article	en