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The Structure and Evolution of Massive Stars
Symposium - International astronomical union
This review is restricted to the most recent studies of the structure of stars in the approximate range from 10 to 100 M⊙, during the core H- and He-burning phases. Other recent major reviews on this subject are by Dallaporta (1971), Massevich and Tutukov (1974) and Iben (1974). The lower limit was chosen to be just above the transition from degeneracy to non-degeneracy in the core at carbon ignition (Schwarzschild and Härm 1958). The upper limit is very uncertain. The canonical value of aboutdoi:10.1017/s0074180900145772 fatcat:4qyn22m2lbganb4c4zk3t5lbva