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- W55807772 abstract "UBV(RI) c and Stromgren photometry has been carried out on a sample of 29 classical T Tauri stars for which a wide range of mass-loss rates has been reported in the literature. We measured their brightness variability in the 3400–8000 A and 3400–5600 A wavelength ranges during observing runs between 7 and 14 days long. To this sample we added other stars for which this information was taken from the literature. We found a correlation between the amplitude of the brightness variability and the strength of the mass-loss process." @default.
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- W55807772 date "1998-01-01" @default.
- W55807772 modified "2023-10-16" @default.
- W55807772 title "Hot Spots on Classical T Tauri Stars with High Mass-Loss Rates" @default.
- W55807772 cites W1980100166 @default.
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- W55807772 doi "https://doi.org/10.1007/978-3-540-68597-5_38" @default.
- W55807772 hasPublicationYear "1998" @default.
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