摘要
This is a review talk. The first part of the talk is to introduce briefly the evolutionary picture of stars with various mass after hydrogen burning. The second one of the talk is about some important physical factors affected on the stellar evolution. The content of the second part of the talk is as follows: A) Physics controlling nuclear burning in the stars 1. Ignition temprature of nuclear burning 2. Lower limit on the core mass of stars for igniting nuclear
