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Magnetic Field Topology of Accreting White Dwarfs

Published online by Cambridge University Press:  12 April 2016

Klaus Reinsch ,
Fabian Euchner ,
Klaus Beuermann  and
Stefan Jordan
Klaus Reinsch
Affiliation:
Universitäts-Sternwarte, Geismarlandstr. 11, 37083 Göttingen, Germany
Fabian Euchner
Affiliation:
Universitäts-Sternwarte, Geismarlandstr. 11, 37083 Göttingen, Germany
Klaus Beuermann
Affiliation:
Universitäts-Sternwarte, Geismarlandstr. 11, 37083 Göttingen, Germany
Stefan Jordan
Affiliation:
Institut für Astronomie und Astrophysik, Eberhard-Karls-Universität Tübingen, Sand 1, 72076 Tübingen, Germany

Abstract

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We 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 HE 1045-0908 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.

Information

Type
Part 2. Magnetic Fields
Information
International Astronomical Union Colloquium , Volume 190: Magnetic Cataclysmic Variables , 2004 , pp. 71 - 77
Copyright
Copyright © Astronomical Society of the Pacific 2004

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