A fast, robust algorithm for the solution of the equation of state for late-type stellar atmospheres
A fast, but accurate procedure to solve the equation of state for late-type stellar atmospheres is an essential component of a realistic model atmosphere code. This requires the determination of the chemical equilibrium of a gas containing significant amounts of perhaps one to two hundred species, o...
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| Language: | English |
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2010
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| Online Access: | http://hdl.handle.net/2429/23881 |