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- W2947488924 abstract "We propose an analytic [Formula: see text] solution of the hydrodynamic equations for a main-sequence star in stationary and spherically symmetric conditions. We reach this result starting from convenient choices of mass density, specific function of the perfect gas, and luminosity function. The theoretical results, when applied to the Sun, are compared with the standard solar model data. A more accurate proof of Schwarzshild’s inequality and equation is given." @default.
- W2947488924 created "2019-06-07" @default.
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- W2947488924 date "2019-08-01" @default.
- W2947488924 modified "2023-09-27" @default.
- W2947488924 title "An analytical solution of stationary hydrodynamic equations of a main-sequence star" @default.
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- W2947488924 doi "https://doi.org/10.1142/s0219887819501202" @default.
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