X-Z Density Contour in Stellar Collapse after nuclear density is reached
Mass = 2.5 solar mass (against Max. of spherical star = 1.60)
Initial Equatorial Radius = 1780 km; Rigid rotation at t=0, T/W=0.0127, q=0.87
Subnuclear density : Γ=1.3 , Above nuclear density : Γ=2.5;
P = Polytropic + Thermal part
