Interim 发表于 2025-3-25 04:09:30

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florid 发表于 2025-3-25 11:21:43

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diathermy 发表于 2025-3-25 12:14:57

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 departur

Osteons 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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神圣在玷污 发表于 2025-3-26 06:56:32

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巩固 发表于 2025-3-26 09:20:44

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转换 发表于 2025-3-26 16:01:59

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串通 发表于 2025-3-26 18:37:06

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查看完整版本: Titlebook: Cosmic Chemistry; Gerhard Klare Conference proceedings 1988 Springer-Verlag Berlin Heidelberg 1988 astrophysics.galaxies.interstellar matt