Speaker
Norhasliza Yusof
(U. of Malaysia)
Description
In the work, we are going to discuss the stellar evolution of Very Massive Stars (M>100 Mo) in different metallicities. This includes the general properties, impact on the chemical abundances due to the rotational impact, dependences in metallicities and mass loss of very massive stars. Very massive stars has very large convective core during the main sequence thus their evolution do not affected by rotational mixing but by the mass loss due to the stellar winds. In the work we also going to discuss the one of the rate of VMS, the pair instability supernovae where we modeled PISN from our VMS progenitor models.
