MOST,Modes and Models

Details MOST,Modes and Models MOST,Modes and Models

Aug 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005jrasc..99..130g&link_type=abstract

Journal of the Royal Astronomical Society of Canada, Vol. 99, No. 4, p.130

Astronomy and Astrophysics

Astronomy

Scientific paper

Stellar model analysis of the first successful seismic observations of a star from space are presented. The low frequency radial p-modes of eta Boo observed by MOST (Microvariability and Oscillations of STars) are used to constrain eta Boo's composition, mass, and age. MOST is a micro-satellite specifically designed to observe parts-permillion luminosity variations in bright stars. The MOST data when combined with ground-based observations imply that the outer layers of our standard models of eta Boo are inaccurate.

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