S. Chandrasekhar, THE MAXIMUM MASS OF IDEAL WHITE-DWARFS, (REPRINTED FROM ASTROPHYSICALJOURNAL, VOL 74, PG 81-82, 1931), Journal of astrophysics and astronomy, 15(2), 1994, pp. 115
The theory of the polytropic gas spheres in conjunction with the equat
ion of state of a relativistically degenerate electron-gas leads to a
unique value for the mass of a star built on this model. This mass (=
0.91.) is interpreted as representing the upper limit to the mass of a
n ideal white dwarf.