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Introduction

Published online by Cambridge University Press:  12 April 2016

M. Takeuti
M. Takeuti*
Affiliation:
Astronomical Institute, Tôhoku University, Sendai 980, Japan

Abstract

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A historical sketch of the nonlinear theory of variable stars is outlined briefly. The main break-through came from the hydrodynamic study of stellar pulsation. From a theoretical point of view, coupling needs to be discussed more carefully. The impact of new opacities on the astrophysical problems is also discussed.

Type
Introduction
Information
International Astronomical Union Colloquium , Volume 134: Nonlinear Phenomena in Stellar Variability , 1993 , pp. 1 - 5
Copyright
Copyright © Kluwer 1993