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Published online by Cambridge University Press: 25 April 2016
The basic system of differential equations governing the non-radial adiabatic oscillations of stars are given in the review article by P. Ledoux and Th. Walraven. The numerical integration of these equations has been undertaken by P. Smeyers and by R. Van der Borght and Wan Fook Sun, in the latter case for stars of uniform composition in the mass range.
where μ is the molecular weight of the stellar material. These integrations were based on models derived by R. Van der Borght.