the density in the stellar center

The influence of the axial rotation on the degenerate dwarfs characteristics

The influence of the axial rotation on degenerate dwarfs characteristics is calculated within the three- and four parametric model.  It was shown that the relative increase of dwarf's mass is about 5%.  Therefore the maximal mass in standard model with paramagnetic electron subsystem reaches $1.52M_\odot$, and in the model with spin-polarized electron subsystem is $2.15M_\odot$.  The dependence of the dwarf's shape was found as a function of the model parameters (the density in the stellar center,  the chemical composition parameter,  the rotation frequency and the degree of polarization).