By S. Chandrasekhar, Kameshwar C. Wali
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Additional resources for A Quest for Perspectives: Selected Works of S. Chandrasekhar: With Commentary (Volume 1)
3°) Comparing (28) and (30), we have w ™--»w*irrf% (3I) or JO 3 Pjjj) = _ PO 3 £
0> 1 -Pe)-curve (see equation (150)). ,). ,) we have centrally condensed configurations on the generalized standard model. main formulae, as the particular form (9) for the equation of state of a perfect gas we are now using has not been used before. We shall confine ourselves to the standard model. (i-^) between the gas and the radiation pressure is a constant. Also in a well-known notation &  • tpcGM (19) The parametric representation for the equation of state in equations (5) and (9) can be used, since " / 3 " is now a constant.
Non-trivial solution when the configuration has a mass less than 2JI, and the value of Milne's fundamental problem lies in this, that without his general formulation it could hardly have been possible to analyse the structure of stellar configurations of mass less than SJt. In this paper a first attempt is made to solve Milne's problem consistent with the exact equation of state for degenerate matter. The analysis has been made possible by the derivation in the previous paper (referred to as I I ) j of the exact differential equation to describe degenerate matter in gravitational equilibrium.
A Quest for Perspectives: Selected Works of S. Chandrasekhar: With Commentary (Volume 1) by S. Chandrasekhar, Kameshwar C. Wali