An exact super dense star model on spheroidal space-time

We consider the 3-dimensional space with t 1 = constant in a super dense star which is spheroidal. We report a class of static spherically symmetric physically viable models based on a particular actual solution of Einsteins field equations. The models of the class admit densities of the order of 2 × 10 14 gm cm − 3 , radii of the order of a few kilometers and maximum masses up to about three times the solar mass.