Host142
发表于 2025-3-25 06:17:20
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Root494
发表于 2025-3-25 08:21:40
Satoshi Yamamotoigt, daß sie die elektromagnetische Wechselwirkung aller geladenen Leptonen mit hoher Präzision beschreibt. Da die Quarks geladene Fermionen sind, lag es nahe, die Formeln der QED auf Streuprozesse, an denen Quarks beteiligt sind, zu übertragen. Darüber hinaus ist die QED das Modell für weitergehend
无意
发表于 2025-3-25 11:42:43
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companion
发表于 2025-3-25 17:50:53
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星球的光亮度
发表于 2025-3-25 23:01:25
Derivation of Molecular Abundances, of thermal radiation and blackbody radiation, a radiative transfer equation is derived and applied for a few ideal cases. A rotation diagram method under a local thermodynamic equilibrium (LTE) condition, a concept of the critical density, and a basic principle of statistical equilibrium calculatio
pacifist
发表于 2025-3-26 00:35:25
Basic Concepts for Gas-Phase Chemical Reactions,ients of chemical reactions are defined both in microscopic and macroscopic views. After summarizing important constraints required for chemical reactions in low-density and low-temperature conditions of interstellar clouds, ion–molecule reactions, neutral–neutral reactions, radiative association re
rectocele
发表于 2025-3-26 04:43:06
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conspicuous
发表于 2025-3-26 09:17:39
Chemistry of Molecular Clouds I: Gas Phase Processes,ity and visual extinction are 10.–10. cm. and higher than a few magnitudes, respectively, and a variety of molecules are detected. This chapter deals with gas-phase chemical reactions in molecular clouds before birth of protostars. In general, interstellar ultraviolet radiation is shielded in molecu
CRAFT
发表于 2025-3-26 14:28:26
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打谷工具
发表于 2025-3-26 17:46:22
Chemistry of Star-Forming Regions,ng regions are summarized, which show significant chemical differentiation within a source as well as among sources. In low-mass star-forming regions, hot corinos characterized by rich saturated organic molecules and warm carbon-chain chemistry sources characterized by rich carbon-chain molecules ar