An abundance analysis for Vega: Is it a lambda Boo star?

Simple item page
dc.creatorIlijic, S.
dc.creatorRosandic, M.
dc.creatorDominis, D.
dc.creatorPlaninic, M.
dc.creatorPavlovski, K.
dc.date1998-05-18
dc.date.accessioned2026-07-07T02:26:58Z
dc.date.available2026-07-07T02:26:58Z
dc.descriptionSince Baschek & Slettebak (1988) drew attention to the similarity between the abundance pattern of lambda Boo stars and that of Vega, there has been a long debate whether Vega should be listed among the chemically peculiar stars of lambda Boo type. We performed an elemental abundance analysis using a high dispersion spectrum in the optical region, and confirmed its mild metal underabundance. In our discussion we reinforce the suggestion that Vega is a mild lambda Boo star.
dc.description3 pages, 1 figure, to appear in: Proc. of the 26th workshop of the European Working Group on CP stars, eds. P. North, A. Schnell and J. Ziznovsky, Contrib. Astr. Obs. Skalnate Pleso Vol. 27, No 3
dc.identifierhttps://arxiv.org/abs/astro-ph/9805234
dc.identifierhttp://arxiv.org/abs/astro-ph/9805234
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12500
dc.subjectAstrophysics
dc.titleAn abundance analysis for Vega: Is it a lambda Boo star?
dc.typetext

Files

Collections

arXiv