Modelling Differential Rotation for Optical Long Baseline Interferometry

Details Modelling Differential Rotation for Optical Long Baseline Interferometry Modelling Differential Rotation for Optical Long Baseline Interferometry

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002sf2a.conf..219d&link_type=abstract

SF2A-2002: Semaine de l'Astrophysique Francaise, meeting held in Paris, France, June 24-29, 2002, Eds.: F. Combes and D. Barret,

Astronomy and Astrophysics

Astrophysics

Scientific paper

Optical long baseline interferometry (OLBI) is a technique sensitive to sky projected brightness distributions, constituting a powerful tool for the study of detailed stellar surface structures. In the present contribution we present a study about the effects of stellar rotation on different interferometric observables through a physically coherent model which includes gravity darkening, geometrical deformation and distinct rotation laws (solid and differential).

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