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Interstellar Molecular Formation Processes,a, the gaseous molecules are exceedingly well characterized and their observation leads to a detailed knowledge of the chemical and physical state of the gas in dense interstellar clouds . For example, gas temperatures are in the range 10 – 70 K and total gas densities are on the order of 10.胆小鬼 发表于 2025-3-25 18:01:38
Nonequilibrium Chemistry in Circumstellar Shells,nstant outflow velocity of 10 km/s, the H. concentration shows the most pronounced departure from kinetic equilibrium caused by the specific temperature-dependence of the main H.-forming reactions and by wind effects. Periodic oscillations of UV radiation and temperature cause a significant departurOsteons 发表于 2025-3-25 21:38:52
Turn Ah-Ha Moments into Pivotal Learning,a, the gaseous molecules are exceedingly well characterized and their observation leads to a detailed knowledge of the chemical and physical state of the gas in dense interstellar clouds . For example, gas temperatures are in the range 10 – 70 K and total gas densities are on the order of 10.除草剂 发表于 2025-3-26 04:06:09
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