Inversion for the internal structure and rotation of the Sun and other sun-like stars

Details Inversion for the internal structure and rotation of the Sun and other sun-like stars Inversion for the internal structure and rotation of the Sun and other sun-like stars

Nov 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998mons.proc...33g&link_type=abstract

The First MONS Workshop: Science with a Small Space Telescope, held in Aarhus, Denmark, June 29 - 30, 1998, Eds.: H. Kjeldsen, T

Physics

5

Scientific paper

Asteroseismic data of the kind accessible to MONS add enormously to the observational information that we can gather about stars. Even simple calibrations of theoretical stellar models based on elementary combinations of oscillation frequencies enable us to refine our knowledge of the interior structure of a star substantially. More sophisticated analyses permit us to proceed further, and to address specific questions that are pertinent to our more general understanding of the structure and evolution of stars.

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