Multi-Element Doppler Imaging of the Ap star epsilon Ursae Majoris

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dc.creatorLueftinger, T.
dc.creatorKuschnig, R.
dc.creatorWeiss, W. W.
dc.date1998-05-19
dc.date.accessioned2026-07-07T02:26:59Z
dc.date.available2026-07-07T02:26:59Z
dc.descriptionThe surface distribution of five elements: iron, chromium, titanium, magnesium and manganese on the magnetic A0pCr star epsilon UMa, have been calculated using the Doppler imaging technique. We found that iron, chromium and manganese are correlated with the assumed dipole magnetic field geometry of this star, which is apparently not the case of magnesium and titanium.
dc.description3 pages, 2 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/9805244
dc.identifierhttp://arxiv.org/abs/astro-ph/9805244
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12503
dc.subjectAstrophysics
dc.titleMulti-Element Doppler Imaging of the Ap star epsilon Ursae Majoris
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