An asymptotic representation of unstable gravity modes in stars

Details An asymptotic representation of unstable gravity modes in stars An asymptotic representation of unstable gravity modes in stars

Dec 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977ap%26ss..52..435d&link_type=abstract

Astrophysics and Space Science, vol. 52, no. 2, Dec. 1977, p. 435-442.

Astronomy and Astrophysics

Astrophysics

2

Asymptotic Methods, Stellar Gravitation, Convection, Series Expansion

Scientific paper

An asymptotic representation is developed for high-order unstable gravity modes in a star, which are associated with a convective zone enclosed between two radiative layers. In the domain which contains both turning points of the differential equation, the solutions are represented by a single asymptotic expansion in terms of Weber functions.

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