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- W1980835640 abstract "Fifteen spectrograms of the Me variable T Arietis were obtained for a study of its spectrum and velocity. The spectral type varies from M6e to M8. Emission lines are present except near minimum, and their behavior is similar to that of the more regular Me stars. XX 3852 Fe I, 3905 Si i, and 3938----? are comparatively strong, while hydrogen emission is weak. The radial velocities from the absorption lines have a range of 8.6 km/sec, but it is not certain that the variation is correlated with phase. The mean velocity is +7.1 km/sec. The mean displacement of the emission lines with respect to the absorp- tion lines (A -E) is +6.5 km/sec, which is about 5 km/sec less than that found for typical Mira variables of the same period" @default.
- W1980835640 created "2016-06-24" @default.
- W1980835640 creator A5007495834 @default.
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- W1980835640 date "1943-11-01" @default.
- W1980835640 modified "2023-10-18" @default.
- W1980835640 title "Spectroscopic Observations of T ARIETIS." @default.
- W1980835640 doi "https://doi.org/10.1086/144574" @default.
- W1980835640 hasPublicationYear "1943" @default.
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