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Physics, 28.09.2019 21:10 manlycool9962

Show that the equation of hydrostatic equilibrium may be written as dps, des where g is the local gravitational acceleration. (this form is useful in models of stellar atmospheres.) use this form to evaluate the pressure at r and estimate the ratio between the centre and surface pressures of a star. for simplicity, assume an average constant opacity for the photosphere.

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