Chandrasekhar, S. (Subrahmanyan), 1910-1995, author.
[Collection of thirty early offprints of journal articles / by Subrahmanyan Chandrasekhar].
Papers by Subrahmanian Chandrasekhar on stellar structure, stellar atmospheres and distorted polytropes. Two papers coauthored with Leon Rosenfeld and Chr. Knakkergr̄d Ml̜ler.
Stars -- Structure.
Stars -- Atmospheres.
Polytropes.
Ml̜ler, Chr. Knakkergr̄d.
Rosenfeld, L. (Leon), 1904-1974.
Professor E. A. Milne on World Structure.
The Ionization-Formula and the New Statistics.
On the Probability Method in the New Statistics.
The Maximum Mass of Ideal White Dwarfs.
The Dissociation Formula According to the Relativistic Statistics.
The Highly Collapsed Configuration of a Stellar Mass.
O2 Eridani B.(Eingegangen am 19. August 1931).
Some Remarks on the State of Matter in the Interior of Stars.
Stellar Configurations with degenerate Cores (1934).
The Highly Collapsed Configurations of a Stellar Mass (Second paper).
Stellar Configurations with Degenerate Cores (1935).
Stellar Configurations with Degenerate Cores (Second paper).
Relativistic Degeneracy.
Stjernernes struktur.
Production of Electron Pairs
The Theory of Stellar Structure.
The Radiative Equilibrium of an Expanding Planetary Nebula.
The Nebulium Emission in Planetary Nebulae.
On the hypothesis of the radial ejection of high-speed atoms for the Wolf-Rayet stars and the nov.̆
The radiative equilibrium of extended stellar atmospheres.
The radiative equilibrium of extended stellar atmospheres-Correspondence.
On the effective temperatures of extended photospheres.
The solar chromosphere.
The relation between the Chromosphere and the Prominences-Correspondence.
The solar chromosphere (Second paper).
An analysis of the problems of the stellar atmospheres.
The equilibrium of distorted polytropes. I. The rotational problem.
The equilibrium of distorted polytropes. II. The tidal problem.
The equilibrium of distorted polytropes. III. The double star problem.
The equilibrium of distorted polytropes. IV. The rotational and the tidal distortions as functions of the density distribution.