Signatures of Convective Cores in Gravity Modes

Details Signatures of Convective Cores in Gravity Modes Signatures of Convective Cores in Gravity Modes

Apr 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..349..297m&link_type=abstract

Astrophysics of Variable Stars, Pecs, Hungary, 5-10 September 2005, Sterken, C. and Aerts, C. (eds). ASP Conference Series, Vol.

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

It is well known that a stratification in the chemical composition of
stars directly influences the properties of gravity modes. As a star
evolves on the main-sequence, a chemical composition gradient develops
at the edge of the convective core. In this work we study the signature
left by such a μ-gradient on the periods of gravity modes.

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