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Spectroscopic and interferometric approach for differential rotation in massive fast rotators
Published online by Cambridge University Press: 12 July 2011
Abstract
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The coupling between the convective region in the envelope and rotation can produce a surface latitudinal differential rotation that may induce changes of the stellar geometry and on the spectral line profiles that it may be scrutinized spectroscopically and by interferometry.
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- Copyright © International Astronomical Union 2011
References
Maeder, A. 2009, Physics, Formation and Evolution of Rotating Stars, (Springer)CrossRefGoogle Scholar
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