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Cold CO in circumstellar disks: On the effects of photodesorption and vertical mixing
ASTRONOMY & ASTROPHYSICS, no. 3.0 (2009): L49-L52
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Aims. We attempt to understand the presence of gas phase CO below its sublimation temperature in circumstellar disks. We study two promising mechanisms to explain this phenomenon: turbulent mixing and photodesorption. Methods. We compute the chemical evolution of circumstellar disks including grain surface reactions with and without turbu...More
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