Structure of the Star with Ideal Gases
arXiv:0712.0219
Abstract
In this paper, we provide a simplified stellar structure model for ideal gases, in which the particles are only driven by gravity. According to the model, the structural information of the star can be roughly solved by the total mass and radius of a star. To get more accurate results, the model should be modified by introducing other interaction among particles and rotation of the star.
9 pages, 5 figures
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