ɛBoo Inversion of simulated rotational profile

Details ɛBoo Inversion of simulated rotational profile ɛBoo Inversion of simulated rotational profile

Apr 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004soph..220..199l&link_type=abstract

Solar Physics, Volume 220, Issue 2, pp.199-205

Physics

5

Scientific paper

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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