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- W3018301923 abstract "We have developed a new method to derive the magnetic field distribution on the surfaces of rotating magnetic white dwarfs from phase-resolved flux and circular polarization spectra. An optimization code based on an evolutionary strategy is used to fit synthetic Zeeman spectra for a variety of model geometries described in the framework of a truncated multipole expansion. We demonstrate that the code allows the reconstruction of relatively complex fields using noise-added synthetic input spectra. As a first application, we analyze flux and circular polarization spectra of the polar EF Eri in a low state of accretion taken with FORS1 at the ESO VLT." @default.
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- W3018301923 date "2003-03-14" @default.
- W3018301923 modified "2023-09-23" @default.
- W3018301923 title "Zeeman tomography of magnetic white dwarfs: General method and application to EF Eridani" @default.
- W3018301923 doi "https://doi.org/10.48550/arxiv.astro-ph/0303336" @default.
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