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Paper: HST/STIS observations of the polar UZ Fornacis in a high state
Volume: 261, The Physics of Cataclysmic Variables and Related Objects
Page: 159
Authors: Nogami, D.; Gänsicke, B. T.; Beuermann, K.
Abstract: We present HST/STIS observations of the polar UZ For obtained during a high state. The ultraviolet and optical spectrum of UZ For can be described by the sum of an optically thin plasma (the accretion stream), a blackbody component (the white dwarf), and cyclotron emission (the accretion column). The detection of cyclotron harmonics in the near-ultraviolet allows a firm determination of the magnetic field strengths of both magnetic poles, B1 = 51 MG and B2 = 74 MG.
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