Hertzsprung-Russel diagram adapted from Costa et al. (2025) showing stars in the LMC. The green and gray lines show tracks from Costa et al. (2025), that were computed with Z = 0.006 and the standard mass-loss rate. The purple and red stars show objects from B22 (red stars indicate R136a), and the blue and red dots are taken from Schneider et al. (2018) (red dots are WNh stars). The dashed pink line and dash-dotted black line show the ZAMS and TAMS, respectively. The zoomed-in plot shows the most massive stars, and the gray shaded region shows the width of the observed temperature range of VMSs in the LMC.