The Constitution of the Stars

Details The Constitution of the Stars The Constitution of the Stars

Sep 1926

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1926natur.118..373g&link_type=abstract

Nature, Volume 118, Issue 2967, pp. 373-374 (1926).

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Scientific paper

ON the theory of radiative equilibrium of stellar interiors, as
developed mainly by Eddington, the assumption appears to be implicit
that the density, mean molecular weight, and other contingent properties
of stellar material, vary in a continuous manner from the star's surface
to its centre. This assumption appears questionable.

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