An automatic procedure for a determination of the effective temperature and gravity - Application to 100 O-type stars
We have developed an automatic procedure to determine Teff and log g from the comparison of observational data with their theoretical values. After a description of the method we compare our results for a sample of 100 O-type stars with the classifications of Conti and Walborn and with the determinations of Morrison by photometric indices. The
Morossi, C. et al.
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9
1980