Stellar disharmony

Abstract

Frequency differences between high-order p-modes of two stellar models, both with the mass and luminosity of the sun, are compared with results of asymptotic theory. The computed relative differences are closely approximated by averages of the relative sound-speed differences, weighted by the local sound travel-time, over the regions where the modes are trapped.

Identifiers

DOI

10.1093/mnras/235.3.875

Citations and references