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 …

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

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 an attempt has been made to determine the effect of Coriolis force on the
shapes of Roche equipotential surfaces of rotating stars and stars in binary systems …

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 …

Abstract Kopal (Adv. Astron. Astrophys. 9: 1–65, 1972) introduced the concept of Roche
equipotentials to incorporate the effects of rotation and tidal distortions on the equilibrium …

In this paper we propose suitable modifications in the concept of Roche equipotentials to
account for the effect of mass distribution inside the star on its equipotential surfaces and …

Abstract Kopal (Adv. Astron. Astrophys., 9, 1, 1972) introduced the concept of Roche
equipotentials to analyse the effects of rotational and tidal distortions in case of stars in …

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 …