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• W3100608524 abstract "Context. In a molecular cloud dust opacity typically dominates over gas opacity, yet in the vicinities of forming stars dust is depleted, and gas is the sole provider of opacity. In the optically thin circumstellar environments the radiation temperature cannot be assumed to be equal to the gas temperature, hence the two-temperature Planck means are necessary to calculate the radiative equilibrium." @default.
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• W3100608524 date "2014-08-01" @default.
• W3100608524 modified "2023-09-23" @default.
• W3100608524 title "Mean gas opacity for circumstellar environments and equilibrium temperature degeneracy" @default.
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• W3100608524 doi "https://doi.org/10.1051/0004-6361/201423768" @default.
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