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 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 …

This paper is based on the method proposed for computing eigenfrequencies of radial
oscillations of some differentially rotating (DR) polytropic stars. It is assumed that stellar …

A systematic way is proposed to determine the balanced structures, equilibria and numerous
physical parameters of differentially rotating polytropic stars taking into the account of the …

In the present thesis an attempt has been made to extend the work of Mohan et al (108, 109)
and Lal (70). This work relates to the analytic studies of the problems of computing the …

The present thesis deals with the problems of determining the effects of differential rotation
on the equilibrium structures of white dwarf stars. This thesis consists of three chapters …

Eigen-frequencies (EF) of non–radial modes (NRM) of pulsations of differentially rotating
(DR) and tidally distorted (TD) stellar models by considering the effect of mass variation (MV) …

In the present paper we have studied the eigenfrequencies of small adiabatic barotropic
pseudo-radial and nonradial modes of oscillations of the white dwarf models of rotating stars …