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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

Cited: 70|Views26

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stars: circumstellar matterstars: planetary systems: protoplanetary disksastrochemistryturbulence

Abstract

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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