Seismic signatures of convective and/or helium cores

Details Seismic signatures of convective and/or helium cores Seismic signatures of convective and/or helium cores

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coast.157..367s&link_type=abstract

Communications in Asteroseismology, Vol.157, p. 367-

Physics

Scientific paper

The ℓ = 0 - ℓ = 2 small separations can become negative in a
certain frequency region during the evolution of solar-type stars. This
specific behaviour can be used to characterize the convective and the
helium stellar cores, and to obtain constraints on the possible extent
of the overshooting at the core edge.

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