Abstract
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. © International Astronomical Union 2011.
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Zorec, J., Frémat, Y., Delaa, O., De Souza, A. D., Stee, P., Mourard, D., … Martayan, C. (2011). Spectroscopic and interferometric approach for differential rotation in massive fast rotators. In Proceedings of the International Astronomical Union (Vol. 6, pp. 103–105). Cambridge University Press. https://doi.org/10.1017/S1743921311010118
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