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Comment on axion emission rates in stars.

It is pointed out that the emission of axions from stellar plasmas and their reabsorption is stimulated by the thermal radiation field in processes with final-state photons. An expression for the bremsstrahlung emissivity of a stellar plasma is given for the nonrelativistic, degenerate regime. Some other aspects of a recent calculation by Pantziris and Kang of stellar axion emissivities are discussed.