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).
- Adams W. S. The spectrum of the companion of Sirius. PASP. 27, 236 (1915).
- Fowler R. H. On dense matter. MNRAS. 87, 114 (1926).
- Chandrasekhar S. The maximum mass of ideal white dwarfs. Astrophys. Journ. 74, 81 (1931).
- Chandrasekhar S. Stellar configurations with degenerate cores' (second paper). MNRAS. 95, 676 (1935).
- Salpeter E. Energy and pressure of a zero-temperature plasma. Astrophys. Journ. 134, 669 (1961).
- Shapiro S. L. Teukolsky S. A. Black Holes, White Dwarfs and Neutron Stars. Cornell University, Ithaca, New York (1983).
- Hamada T., Salpeter E. Models for zero-temperature stars. Europ. Astrophys. J. 133, 683 (1961).
- Zeldovich Ya. B., Novikov I. D. Relativistic astrophysics. Moscow, Nauka (1967).
- Vavrukh M. V., Smerechinskii S. V. A finite temperature Chandrasekhar model: determining the parameters and computing the characteristics of degenerate dwarfs. Astronomy Reports. 56, n.5, 363 (2012).
- Vavrukh M. V., Smerechinskii S. V. Hot degenerate dwarfs in a two-phase model. Astronomy Reports. 57, n.2, 913 (2013).
- Vavrukh M., Tyshko N., Smerechynskyj S. Interparticle interactions, general relativity effects, and critical parameter of white dwarfs. Mathematical Modeling And Computing. 1, n.2, 264 (2014).
- Vavrukh M. V., Dzikovskyi D. V., Tyshko N. L. Model of degenerate dwarf with spin-polarized electron system. Odessa Astronomical Publications, 28, n.1, 82 (2015).