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- W4302415183 abstract "Context. A large number of Be stars exhibit intensity variations of their violet and red emission peaks in their H i lines observed in emission. This is the so-called V/R phenomenon, usually explained by the precession of a one-armed spiral density perturbation in the circumstellar disk. That global-disk oscillation scenario was confirmed, both observationally and theoretically, in the previous series of two papers analyzing the Be shell star ζ Tauri. The vertically averaged (2D) global-disk oscillation model used at the time was able to reproduce the V/R variations observed in Hα, as well as the spatially resolved interferometric data from AMBER/VLTI. Unfortunately, that model failed to reproduce the V/R phase of Br15 and the amplitude of the polarization variation, suggesting that the inner disk structure predicted by the model was incorrect." @default.
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- W4302415183 date "2015-04-01" @default.
- W4302415183 modified "2023-10-11" @default.
- W4302415183 title "2.5D global-disk oscillation models of the Be shell starζ Tauri" @default.
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- W4302415183 doi "https://doi.org/10.1051/0004-6361/201425446" @default.
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