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W1675278671 abstract "We present spin-phase resolved spectroscopy of the nova-like cataclysmic variable (CV) AE Aquarii. Unlike in other magnetic CVs, the pulsed fraction of the Balmer emission line intensities is small and must be below the detection limit of ∼2 %. From the absorption lines of the K star secondary we derive an improved orbital ephemeris which is 180° out of phase with respect to the pulse-timing orbit of Robinson et al. (1990, 1991). Combining their pulse-timing amplitude with the absorption line radial velocity amplitude, we find the mass ratio q=M 2 /M 1 =(0.77±0.03). The most probable masses of the binary components are M 1 =0.91 M ○. and M 2 =0.70 M ○. giving an inclination i=57°" @default.
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W1675278671 date "1994-02-01" @default.
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W1675278671 title "Spin-phase resolved optical spectroscopy of AE Aquarii" @default.
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