Abstract
Modelling of polarized cyclotron emission from magnetic cataclysmic variables has been a pivotal technique for determining the structure and location of the accretion zones on the white dwarf. Stokes imaging of Potter et al. [8] is the first objective and analytical technique that robustly models the cyclotron emission and maps the accretion zones.
Polarisation modelling is discussed, followed by a summary of the Stokes imaging technique. We demonstrate this technique on new polarimetric observations of the magnetic cataclysmic variable V834 Cen.
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Potter, S., Romero-Colmenero, E., Buckley, D., Cropper, M., Hakala, P. (2001). Stokes Imaging of the Accretion Region in Magnetic Cataclysmic Variables. In: Boffin, H.M., Cuypers, J., Steeghs, D. (eds) Astrotomography. Lecture Notes in Physics, vol 573. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-45339-3_17
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DOI: https://doi.org/10.1007/3-540-45339-3_17
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