Chemical Characteristics of Embedded Young Stellar Objects
作者： Michiel R. Hogerheijde
DOI: 10.1017/S0074180900164691
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摘要: Based on theoretical considerations, the chemistry around embedded young stellar objects is expected to be governed by interplay between gas-phase reactions, condensation of molecules onto dust grains, grain surface and evaporation altered ice mantles near star in outflow. I discuss chemical characteristics objects, with special emphasis these processes.
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