Analytic stellar structure

Details Analytic stellar structure Analytic stellar structure

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ap%26ss.197..153h&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 197, no. 1, p. 153-161.

Physics

Stellar Interiors, Stellar Models, Stellar Structure, Energy Conservation, Hydrostatics, Stellar Physics

Scientific paper

This paper continues to elaborate on analytic methods to construct models for the internal structure of solar-type stars. Since a detailed stellar model is desired, a nonlinear analytic density distribution in terms of a two-parameter family of models has been assumed. Hydrostatic equilibrium and energy conservation determine the conditions in the gravitationally stabilized stellar fusion reactor. The results show once more that methods of differential and integral calculus provide a laboratory for the application of special functions of mathematical physics in stellar structure.

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