THE INFLUENCE OF THE RADIATION PRESSURE IN THE BINARY W UMi SYSTEM, USING THE POPOVICI MODEL

摘要

The model of the motion of a silicon particle under the influence of gravity and radiation pressure in the W UMi binary system is presented using the C-tin Popovici Model. We will determine the β1 and β2 ratios from the two luminous bodies and we will study the equilibrium points, including those outside the orbital plane.