  Massive stars unable to sustain gravitational collapse, at the end of nuclear
burning stage, turns out into core-collapse supernovae, leaving behind compact
objects like neutron stars or black holes. The progenitor properties like mass
and metallicity primarily governs the explosion parameters and type of compact
remnant. In this contribution we summarize observational study of three Core
Collapse type IIP SNe 2012aw, 2013ab and 2013ej, which are rigorously observed
from ARIES and other Indian observatories and discuss their progenitor and
explosion properties.
