Stripped envelope supernovae (SE-SNe) comprises the group of Type IIb, Ib and Ic SNe. One or more phases of mass transfer or a common envelope evolution can remove the hydrogen or helium envelope. Such stripped stars are considered as progenitors of Type Ib and Ic SNe while binary evolution scenario involving a common envelope phase may be considered as progenitor of SNe IIb sub-types. Different mechanisms driving these progenitor scenario depending upon the orbital parameters and seperation between the components will be discussed in this talk. We will also discuss how observationally the evidence of different mass progenitors can be inferred along with some examples.