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Theoretical Stellar Energy Distributions
Published online by Cambridge University Press: 30 March 2016
Summary
We are working hard to improve model atmospheres because existing models have numerical errors, an unphysical treatment of convection, an inadequate or non-existant treatment of statistical equilibrium, an arbitrarily chosen microturbulent velocity, an arbitrarily chosen helium abundance, and a greatly underestimated line opacity for iron group elements.
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- Synthetic Photometry
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- Copyright © Reidel 1986
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