Abstract
The detection of solar oscillations on ηBoo is now established. We explore here what we can expect from the inversion of similar data by COROT to recover the rotational profile of the star. We show that the observation of a few low-l mixed modes in the excited high frequency range gives access to the rotational gradient if it is large enough.
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Lochard, J., Samadi, R. & Goupil, MJ. ηBoo Inversion of simulated rotational profile. Solar Physics 220, 199–205 (2004). https://doi.org/10.1023/B:SOLA.0000031376.55932.b6
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DOI: https://doi.org/10.1023/B:SOLA.0000031376.55932.b6