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Lecture 1 Time Scales, Temperature-density Scalings, Critical Masses

Lecture 1 Time Scales, Temperature-density Scalings, Critical Masses. I. Preliminaries. The life of any star is a continual struggle between gravity, seeking to reduce the star to a point, and pressure, which supports the star. Stars are gravitationally confined thermonuclear reactions.

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Main sequences stars - PowerPoint PPT Presentation

Lecture 1 Time Scales, Temperature-density Scalings, Critical Masses