Rotational inversion for selected solar-like stars

Details Rotational inversion for selected solar-like stars Rotational inversion for selected solar-like stars

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004sf2a.conf..299l&link_type=abstract

SF2A-2004: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 14-18, 2004. Edited by F. Combes, D. Barret

Astronomy and Astrophysics

Astrophysics

Scientific paper

We show from artificial data that it is possible to invert in rotation
solar-like oscillations for specific stars. We place ourselves in the
COROT mission framework and proceed to a rigorous mode selection. The
rotational splittings are inverted for different conditions ranging from
the ideal to more realistic cases.

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