1. Numerical calculations give the following values for the central temperature and density as a function of mass for ze
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1. Numerical calculations give the following values for the central temperature and density as a function of mass for ze
1. Numerical calculations give the following values for the central temperature and density as a function of mass for zero-age main sequence stars: 50 Msun (log Tc, log pe) = (7.6,0.3) 10 Msun (log Tc, log pe) = (7.5, 0.8) 1 Msun (log Tc, log pe) = (7.2, 2.0) 0.1 Msun (log Te, log pe) = (6.6, 2.8) Compare the three components of the pressure (radiation pressure, ideal gas, and pressure for a fully degenerate gas) assuming full ionization and a pure hydrogen gas for all four masses (you can use the relevant equations from the summary in the notes).
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