Article contents
Radial Oscillations of Stellar Models: Density Distributions which Lead to Three-term Recurrence Relations
Published online by Cambridge University Press: 25 April 2016
Extract
In an early paper Sterne investigated the pulsational properties of three stellar models with specified density distributions. He assumed a solution for the relative amplitude of the displacement to be of the form and on substitution into Eddington’s equation for small radial adiabatic oscillations of a star obtained a two-term recurrence relation to solve for the an in the case of each model.
- Type
- Contributions
- Information
- Publications of the Astronomical Society of Australia , Volume 1 , Issue 7 , April 1970 , pp. 328 - 329
- Copyright
- Copyright © Astronomical Society of Australia 1970
References
- 1
- Cited by