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).