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- W1981641114 abstract "Results of single-trailed spectrograms of the magnetic accreting white-dwarf binary 0139 - 68 are presented. The spectral resolution is approximately 2.5 A and the time resolution is 45 seconds. Line-profile changes and radial velocities are derived and described. A discussion of possible orbital velocities indicates probable masses of 0.2-0.6 solar mass for the white-dwarf primary and 0.3 solar mass for the M-star secondary. The position of the active pole is suggested. The origin of the high-velocity line components is not clear, but their behavior is similar to those in the system VV Pup." @default.
- W1981641114 created "2016-06-24" @default.
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- W1981641114 date "1985-05-01" @default.
- W1981641114 modified "2023-09-27" @default.
- W1981641114 title "Continuous time-resolved spectroscopy of the AM Herculis binary 0139 - 68" @default.
- W1981641114 doi "https://doi.org/10.1086/131555" @default.
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