The distribution of physical parameters and abundances of a 0.1 M_⊙/yr model just before the end of evolution. Left panel: Log T versus log R plot for the 0.1 M_⊙/yr model at the end of its evolution upon encountering GR instability at a mass of 108 000 M_⊙. The blue zones indicate convective zones and grey zones correspond to radiative zones. The enclosed mass is indicated at different radii (see the numbers at red points). Most of the mass (105 000 M_⊙) is within a radius of 10¹³ cm or 14.0 R_⊙ that represents 1% of the total radius. Only a fraction of mass (still 23 000 M_⊙) in the outer envelope implying the star is extremely bloated. Right panel: The plot depicts the change in abundance of various elements inside the 0.1 M_⊙/yr model upon encountering the GR instability when central mass fraction of hydrogen is 0.244.