Asymptotic representation of nonradial g^+^-modes in stars with a convective core.

Details Asymptotic representation of nonradial g^+^-modes in stars with a convective core. Asymptotic representation of nonradial g^+^-modes in stars with a convective core.

Feb 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...318...99w&link_type=abstract

Astronomy and Astrophysics, v.318, p.99-107

Astronomy and Astrophysics

Astrophysics

3

Stars: Oscillations, Stars: Interiors, Methods: Analytical

Scientific paper

The asymptotic representation of linear, isentropic, low-frequency g^+^-modes in spherically symmetric stars developed by Smeyers et al. (1995A&A...301..105S) is extended to more realistic stellar models composed of a convective core in adiabatic equilibrium and a radiative envelope. By means of a boundary-layer method, it is taken into account that the transition from the convective core to the radiative envelope is a turning point for one of the governing differential equations in the divergence and the radial component of the Lagrangian displacement.

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