Two spherical stars A and B have densities PA and PB, respectively. A and B have the same radius, and their masses M and M are related by MB = 2 MA. Due to an interaction process, star A loses some of its mass, so that its radius is halved, while its spherical shape is retained, and its density

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Two spherical stars A and B have densities PA and PB, respectively. A and B have the same radius, and their masses M₁ and M³ are related by MB = 2 MA. Due to an interaction process, star A loses some of its mass, so that its radius is halved, while its spherical shape is retained, and its density remains PA. The entire mass lost by A is deposited as a thick spherical shell on B with the density of the shell being PA. If VA and VÅ are the escape velocities from A and B after the interaction process, the ratio 10n The value of n is 151/3 VA =

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