分子气体的英文

• molecular gas

• "分子"英文翻译    numerator molecule
• "气体"英文翻译    gas; gaseous fluid
• "分子气体常数" 英文翻译 :    gas constant per molecule
• "分子气体激光" 英文翻译 :    molecular gas laser
• "分子气体激光器" 英文翻译 :    molecular gas laser
• "克分子气体常数" 英文翻译 :    molar gas constant; molecular gas constant
• "单原子气体" 英文翻译 :    monatomic gas; monoatomic gas
• "等离子气体" 英文翻译 :    plasma gas
• "电子气体" 英文翻译 :    electron gas
• "多原子气体" 英文翻译 :    polyatomic gas
• "二原子气体" 英文翻译 :    diatomic gas
• "光子气体" 英文翻译 :    photon gas
• "核子气体" 英文翻译 :    nucleon gas
• "离子气体" 英文翻译 :    ionized gas
• "双原子气体" 英文翻译 :    diatomic gas
• "中子气体" 英文翻译 :    neutron gas
• "中子气体靶" 英文翻译 :    neutron gas target
• "质子气体模型" 英文翻译 :    proton gas model
• "等离子气体进口" 英文翻译 :    plasma gas inlet
• "等离子气体显示器" 英文翻译 :    gas plasma display
• "二原子气体激光器" 英文翻译 :    diatomic molecules gas laser
• "离子气体激光器" 英文翻译 :    ion gas laser
• "热离子气体二极管" 英文翻译 :    rectigon
• "原子气体激光器" 英文翻译 :    atomic gas laser
• "自由质子气体模型" 英文翻译 :    free proton gas model

• This circumstance means that cool molecular gas is located there, a vestige of the original gas-dust cloud from which not massive stars were formed, spawning hii zones .
  这种情形意味着那里有冷分子气体，它是形成大质量高温星、产生H区的原始气尘云残余。
• Excimer lasers are produced by means of activating the quasimolecule
  准分子激光是以准分子气体作为激活介质而产生的激光。
• This circumstance means that cool molecular gas is located there , a vestige of the original gas - dust cloud from which not massive stars were formed , spawning hii zones
  这种情形意味着那里有冷分子气体，它是形成大质量高温星、产生h区的原始气尘云残余。
• Besides acting as powerful signposts of active star formation , the intense maser emission provides a unique tool to probe the physical conditions and kinematics of these regions on scales of 10 - 103 au
  星际脉泽不仅是恒星形成的一个及其重要的标志，而且也提供围绕大质量恒星尺度10 - 10 ~ 3au分子气体的物理条件和动力学结构的信息。
• The pyrolysis mechan ism functions of the second stage of dvb / hpso and vpso / hpso are both parabola principle , and the rates of pyrolysis reactions in this stage are both controlled by one - dimensional diffusion
  600时， ai可与先驱体裂解产生的含碳小分子气体反应生成a14c3 ， 800时ai可与裂解气氛nz反应生成ain ，温度升高， al的氮化反应不断进行。
• We have analyised the observed results of low and high spatial resolution observations of molecular line emission toward regions of high - mass star formation which have contributed to the understanding of the physical conditions , morphologies , and dynamics of the molecular gas in the immediate vicinity of recently formed massive stars
  本文研究了来自大质量恒星形成区的一些分子谱线的低分辨率和高分辨率观测结果。这些结果有助于我们了解在最近形成的大质量恒星附近分子气体的物理条件，形态以及动力学结构。