Statistical Distribution of the Formation of Compact Objects in the Milky-Way Galaxy

Abstract

The issue of galactic dynamism and structure is one of the top astrophysical research area. There is a progress both theoretically and observationally. Here, we examined one of the standard statistical approach called the initial mass function to population density to determine the population of newly formed compact objects in the Milky-Way galaxy. To this model we imposed an oversimplifying condition where the formation region is as a system assumed to be of spherical symmetry with falling density outward radially. The result is just in agreement with observation. But here we questioned the existing models are so oversimplified to be further developed.