Solar-like stars as seen by CoRoT

Details Solar-like stars as seen by CoRoT Solar-like stars as seen by CoRoT

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.157..288g&link_type=abstract

Communications in Asteroseismology, Vol.157, p. 288-289

Physics

2

Scientific paper

For more than a year, photometric high-quality data have been achieved from the CoRoT (COnvection ROtation and Planetary Transits; Baglin et al. 2006, Michel et al. 2008) min- isatellite developed by the French space agency (CNES) in collaboration with the Science Program of ESA, Austria, Belgium, Brazil Germany and Spain. The power spectrum of 4 dif- ferent solar-like stars (stars having sub-surface convective zones showing an acoustic (p) mode spectrum) has been obtained with unprecedented quality allowing the precise study of their seismic properties. These solar-like stars are F stars with masses in the range 1.0 to 1.4 M&sun; and are significantly hotter than the Sun.

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