While studying mass transfer in binary star systems, I came across the concept of Roche lobes and the role of the inner Lagrangian point $L_1$, as shown in the adjoining figure.
However, I am having a doubt in understanding the reason of the fact that one lobe is larger and the other is smaller. I think that the reason is due to the different masses of the two stars. Since the contours are equipotentials, it seems that larger the mass of a star, the larger is the size of the corresponding lobe. But I am not sure whether this is the exact reason.
So, I am looking for a proper reason for the different sizes of the two lobes.