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- W48819022 abstract "From phase-resolved spectroscopy around Hβ and Hγ we derive a secure orbital period of 0.24507(20) days. We report the discovery of narrow Balmer emission-line components from the heated hemisphere of the secondary facing the white dwarf. Combined with the Balmer absorption lines from the accretion disk, the system effectively becomes a double-lined spectroscopic binary. The mass ratio is q=M 1 /M 2 =1.35±0.10. The inclination is between i=28° and ∼40° and is not sufficiently constrained to derive accurate masses. The distance of RW Sex is d∼150 pc and its absolute magnitude M v ∼4.8" @default.
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- W48819022 date "1992-03-01" @default.
- W48819022 modified "2023-10-18" @default.
- W48819022 title "Phase-resolved spectroscopy of the novalike cataclysmic variable RW Sextantis." @default.
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