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Iteration Stability for Simple Newtonian Stellar Systems

By Richard Price and others
For an equation of state in which pressure is a function only of density, the analysis of Newtonian stellar structure is simple in principle if the system is axisymmetric, or consists of a corotating binary. It is then required only to solve two equations: one stating that the "injection energy",... Show more
March 18, 2009
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Iteration Stability for Simple Newtonian Stellar Systems
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