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- W5846979 abstract "RW Aur is one of the most active T Tau-type stars with essentially variable emission line spectrum. In order to study the nature of this variability, patrol spectroscopic observations of the star were carried outfrom November 1979 to March 1982 at the 2.6-meter telescope of the Crimean Astrophysical Observatory. The spectral region λ3800–6700 A has been observed with a dispersion of about 40 A/mm. All nights were supplied with simultaneous spectrophotometry of the star.KeywordsRadial VelocityLine ProfilePeriodic VariationAstronomical LetterProbable PeriodThese keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves." @default.
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- W5846979 date "1983-01-01" @default.
- W5846979 modified "2023-09-27" @default.
- W5846979 title "Quasi-Periodic Variations of Balmer Line Profiles in Spectra of the T Tau-Type Star RW Aurigae" @default.
- W5846979 doi "https://doi.org/10.1007/978-94-009-7157-8_74" @default.
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