The Roche Problem: And Its Significance for Double-Star Astronomy / Edition 1

by Zdenek Kopal

Overview

The words of this preface were written when the book was ready to go to the press; and are limited to only a few points which are best made in this place. As is intimated by the sub-title, the whole volume was written with applications in mind to double-star astronomy. The latter is, however, not the only branch of our science which could benefit from its contents. The same is true of certain aspects of the dynamics of stellar systems or galaxies (the stellar populations of which are also characterized by the fact that the mean-free-path of their constituent stars are long in comparison with the dimensions of the respective systems); the central condensations of which are high enough to approximate the gravitational action of a "mass-point". This fact did not, to be sure, escape the attention of previous investigators (in the case of globular clusters, in particular, the Roche model was introduced in their studies under the guise of polytropic models characterized by the index n = 5); though no particular attention will be paid to these in this book. But possible applications of the Roche model are not limited to problems arising in stellar astrophysics. With Coulomb forces replacing gravitation, the equilibrium model finds a close analogy in the field of electrostatics-as was pointed out already at the beginning of this century by (then young) J. H. Jeans (cf.

Product Details

ISBN-13:	9780792301295
Publisher:	Springer Netherlands
Publication date:	02/28/1989
Series:	Astrophysics and Space Science Library , #152
Edition description:	1989
Pages:	264
Product dimensions:	6.10(w) x 9.25(h) x 0.03(d)

Table of Contents

List of Contents.- I. Introduction.- I.1 Bibliographical Notes.- II. The Roche Model.- II.1 Roche Model—A Definition.- II.2 Geometry of Roche Equipotentials.- II.3 Time-Dependent Roche Equipotentials.- II.4 Bibliographical Notes.- III. Roche Coordinates.- III.1 Metric Transformations.- III.2 Equations of Motion in Roche Coordinates.- III.3 Bibliographical Notes.- IV. Continuous Mass Distribution: Clairaut’s Theory.- IV.1 Equipotential Surfaces.- IV.2 Rotational Distortion.- IV.3 Tidal Distortion.- IV.4 Interaction Between Rotation and Tides.- IV.5 Effects of Internal Structure.- IV.6 Bibliographical Notes.- V. Clairaut Coordinates.- V.1 Metric Transformation.- V.2 Internal Structure.- V.3 Vibrational Stability.- V.4 Bibliographical Notes.- VI. Generalized Rotation.- VI.1 Equations of Motion for Deformable Bodies.- VI.2 Dissipative Forces: Effects of Viscosity.- VI.3 Precession and Nutation of Deformable Bodies.- VI.4 Bibliographical Notes.- VII. Observable Effects of Distortion in Close Binary Systems.- VII.1 Radiative Transfer in Clairaut Coordinates.- VII.2 Light Variations in Close Binary Systems.- VII.3 Light Changes of Distorted Systems Within Eclipses.- VII.4 Radial Velocity Variations in Close Binary Systems.- VII.5 Bibliographical Notes.- References.

Editorial Reviews

On the application of the Roche model to double-star astronomy. The model, however, also applies to aspects of the dynamics of stellar systems or galaxies. Also, due to similarities between gravitational and electrostatic effects, the model finds a close analogy in the field of electrostatics, and possibly in other domains beyond the limits of classical astronomy. Although the model is named after the nineteenth-century French mathematician Edward Albert Roche, the problems confronted by the model go back as far as astronomy in the age of Newton. For scholars in astronomy or astrophysics. Acidic paper. Annotation c. Book News, Inc., Portland, OR (booknews.com)

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