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- W47445630 abstract "The T Tauri star RY Lupi was followed simultaneously spectroscopically and photometrically over 7 nights covering one of its deepest brightness minima ever recorded. As reported earlier the star first becomes redder with decreasing brightness. At V = 12.5 this trend is changed towards the blue and this time the object was as blue as in maximum at the deepest minimum. The spectral type (G8) remains constant over the entire range of 3 mag in V. During the deep minimum, when the star brightened from V = 13. 12 to V = 12.45, the line-to-continuum ratios and equivalent widths of absorption features in the U- and B-bands did not change with time" @default.
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- W47445630 date "1993-11-01" @default.
- W47445630 modified "2023-09-27" @default.
- W47445630 title "The circumstellar gleam from the T Tauri star RY Lupi" @default.
- W47445630 hasPublicationYear "1993" @default.
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