iota Cas: Multi-element Doppler imaging and magnetic field geometry

Simple item page
dc.creatorKuschnig, R.
dc.creatorWade, G. A.
dc.creatorHill, G. M.
dc.creatorPiskunov, N.
dc.date1998-05-19
dc.date.accessioned2026-07-07T02:26:59Z
dc.date.available2026-07-07T02:26:59Z
dc.descriptionIn order to clarify the role of the magnetic field in generating abundance inhomogeneities in the atmospheres of Ap stars, we present new abundance Doppler images and an approximate magnetic field geometry for the Ap star iota Cas.
dc.description3 pages, 2 figures, 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/9805243
dc.identifierhttp://arxiv.org/abs/astro-ph/9805243
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12502
dc.subjectAstrophysics
dc.titleiota Cas: Multi-element Doppler imaging and magnetic field geometry
dc.typetext

Files

Collections

arXiv