Pre-main sequence evolution and the chemical structure of MS stars |
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| Authors: | M. Moretti |
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| Affiliation: | (1) Laboratorio di Astrofisica Spaziale, CNR, Frascati, Italy |
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| Abstract: | Pre-Main Sequence evolution has been revised in the light of the present improved knowledge of several physical mechanisms. A good agreement is found with previous computations. Comparison with the  relaxation method (Caloiet al., 1967) shows that such a procedure is also able to give minor characteristics of the chemical distribution in MS-structures. |
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