论文部分内容阅读
晋煤集团煤化工产业发展思路
【机 构】
：
晋煤集团 煤化工研究院
【出 处】
：
第十八届全国气体净化及硫磺回收技术年会
【发表日期】
：
2017年期
其他文献
Outline 1 Background and Motivation 2 Dynamical State of B68 3 Collisional shock waves heating the core?
会议
Background ：Why HLC？. Observation : HSVMT 27、GEMINI. Discussion & Outlook.Infrared cirrus Low et al. 1984. CO molecular clouds : Blitz etal.1984 ,Heithausen et a
Outline Introduction Sample and archival data Classification Results and discussions Summary
会议
Introduction Introduction Observations of star forming regions and cool gas in far InfraRed Star formation and evolution of galaxies
会议
Regulated Star formation efficiency in MW Regulating star formation:gravity+Turbulence+or-Magnetic fields-feedback of massive stars+or-
会议
Motivation Astrochemical simulation is a tool to simulate the time-dependent chemical evolution of various molecular species of cold cores,collapse cores,et al.
Introduction:Methanol masers(class Ⅰ and Ⅱ) Class Ⅰ masers are usually associated with outflows,spread over～10"
会议