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- W2091255343 abstract "From a set of high-resolution spectral observations of late type giant stars we used Doppler imaging to derive time-series temperature maps of the stellar surfaces. Using these temperature maps, it is possible to track the temporal changes of the spot features and derive estimates of the strength and sign of the differential surface rotation of these stars. Looking into the latitudinal changes of the surface maps, it is also possible to derive meridional flows on these stars. But due to the lower accuracy of the latitudes of the reconstructed spot features, the data requirements are higher than for the detection of differential rotation. Nevertheless, a correlation between the differential rotation and meridional flow estimates is suggested. (© 2007 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim)" @default.
- W2091255343 created "2016-06-24" @default.
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- W2091255343 date "2007-12-01" @default.
- W2091255343 modified "2023-10-14" @default.
- W2091255343 title "Differential rotation of giant stars" @default.
- W2091255343 cites W2072538366 @default.
- W2091255343 doi "https://doi.org/10.1002/asna.200710869" @default.
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