The incidence of nonradial pulsation in the lambda Bootis stars

dc.creatorBohlender, D. A.
dc.creatorGonzalez, J. -F.
dc.creatorMatthews, J. M.
dc.date1998-05-18
dc.date.accessioned2026-07-07T02:26:58Z
dc.date.available2026-07-07T02:26:58Z
dc.descriptionWe have completed a high-resolution, high-signal-to-noise, spectroscopic survey of the northern members of the peculiar lambda Boo stars in order to investigate the frequency of the incidence of nonradial pulsation (NRP) in these metal-deficient stars. Of 18 objects observed, 9 show conclusive evidence of NRP, which suggests that pulsation instability is a common phenomenon in the lambda Boo class.
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/9805227
dc.identifierhttp://arxiv.org/abs/astro-ph/9805227
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12494
dc.subjectAstrophysics
dc.titleThe incidence of nonradial pulsation in the lambda Bootis stars
dc.typetext

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