Investigating star-formation activity towards the southern HII region RCW 42
Massive stars (M ≳ 8 Msun) play an important role in the evolution of the interstellar medium due to their high energy output, supernovae explosions, and enrichment of the surrounding medium by heavy elements. The formation of these stars can be studied through the HII regions formed due to the increased output of UV photons from them. Moreover, a multiwavelength study of the molecular clouds associated with these HII regions gives important clues about the evolutionary stages of star-formation.
