The Hertzsprung-Russel diagram is shown for several evolutionary models (LMC) with initial masses from 9 to 30 M_⊙ and surface rotational velocities of approximately 200 km s^-1. Additionally, our sample with LMC-metallicity is depicted. Stars of Class 1 are indicated by circles and stars of Class 2 are represented by triangles. With respect to Fig. 8, stars in Box 1 are shown in red, star in Box 3 in blue and stars in Box 5 in black. Grey dots depict the remaining not analyzed stars of the VLT-FLAMES Survey (LMC) after the selection criteria applied in Brott et al. (2011b).