Magnetic field topology of accreting white dwarfs

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dc.creatorReinsch, Klaus
dc.creatorEuchner, Fabian
dc.creatorBeuermann, Klaus
dc.creatorJordan, Stefan
dc.date2003-02-04
dc.date.accessioned2026-07-07T02:07:28Z
dc.date.available2026-07-07T02:07:28Z
dc.descriptionWe report first results of our systematic investigation of the magnetic field structure of rotating single magnetic white dwarfs and of white dwarfs in magnetic cataclysmic variables. The global magnetic field distributions on the isolated white dwarf HE1045-0908 and the accreting white dwarfs in EF Eri and CP Tuc have been derived from phase-resolved flux and polarization spectra obtained with FORS1 at the ESO VLT using the systematic method of Zeeman tomography.
dc.description8 pages, 9 figures, due to the size limit the resolution of the original figures is higher than in this preprint
dc.identifierhttps://arxiv.org/abs/astro-ph/0302056
dc.identifierhttp://arxiv.org/abs/astro-ph/0302056
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5705
dc.subjectAstrophysics
dc.titleMagnetic field topology of accreting white dwarfs
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