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Published byJacob Knight Modified over 9 years ago
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Stephen Potter South African Astronomical Observatory Polarization studies of magnetic Cataclysmic Variables
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Outline Photo-polarimetry Model to derive shock geometry Doppler tomography => overall accretion geometry Spectropolarimetry Investigate the shock structure Future with SALT Spectropolarimetry with PFIS
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SAAO 1.9m
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Stokes imaging Potter et al (2004) MNRAS 248, 316
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Doppler tomography Potter et al (2004) MNRAS 348, 316
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QS Tel trailed spectra Schwope et al. 1995 A&A 293, 764 ESO/MPI 2.2m
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QS Tel trailed spectra Schwope et al. 1995 A&A 293, 764 ESO/MPI 2.2m
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QS Tel average spectra Schwope et al. 1995 293, 764 ESO/MPI 2.2m
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V834 Cen spectropolarimetry Wickramasinghe Tuohy & Visvanathan ApJ 318, 326 AAT 3.9m
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V834 Cen spectropolarimetry Wickramasinghe Tuohy & Visvanathan ApJ 318, 326 AAT 3.9m
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Spectropolarimetry of AM Her Schaich et al. 1992 A&A 264, 529 2.2m German/Spanish Calar Alto
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Spectropolarimetry with SALT
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Shock models Wickramasinghe & Meggitt 1982 MNRAS 198, 975
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Stratified accretion shock models Potter et al (2002) ASPC, 261, 165
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