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- W20341206 abstract "The technique of back-projection Doppler tomography has been used to produce the first set of reconstructed images of chromospheric emission sources in the class of Algol-type binaries. The Hα emission sources in the Doppler tomograms include the gas stream, a sub-Keplerian accretion annulus, a quasi-stable accretion disk, and the chromosphere of the cool secondary star. The chromospheric images of several Algol secondaries (e.g., RS Vul, β Per, TX UMa, RW Tau) are consistent with that of the RS CVn binary V711 Tau." @default.
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- W20341206 date "1996-01-01" @default.
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- W20341206 title "Doppler tomography of chromospheres and accretion regions in Algol binaries" @default.
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- W20341206 doi "https://doi.org/10.1017/s0074180900083510" @default.
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