We consider a synchronized, circular-orbit binary consisting of a polytrope with index n and
a point-mass object, and use a self-consistent field (SCF) method to construct the …

We propose suitable modifications in the concept of Roche equipotentials to account for the
effect of mass distribution inside a star. The Kippenhahn and Thomas (1970) approach is …

In the present paper we have considered the problem of determining the equilibrium
structure of differentially rotating stars in which the angular velocity of rotation varies both …

A method is proposed for determining equilibrium structures and various physical
parameters of differentially rotating polytropic models of stars, taking into account the effect …

A method is proposed to compute the eigenfrequencies of small adiabatic pseudo-radial
modes of oscillations of differentially rotating and tidally distorted stellar models by taking …

Abstract The original Strum-Liouville type of equation is tuned suitably to study the
pulsational properties of gaseous spheres of non-uniform densities from centre to surface …

The concept of Roche equipotentials has been frequently used in literature to study the
problems of rotating stars and stars in binary systems. However in spite of using this …

In this paper a method is proposed for computing the equilibrium structures and various
other observable physical parameters of the primary components of stars in binary systems …

In this paper we propose a method for computing the equilibrium structure and various
physical parameters of differentially rotating and tidally distorted polytropic stars. The law of …

In this paper the approach of Mohan and Saxena (for instance see: C. Mohan and RM
Saxena; Effect of rotation and tidal distortion on the periods of small adiabatic oscillations of …