dusty-gas 含灰气体
dusty-gas model 尘气模型
dusty-gas shock tube 含灰气体激波管
dusty-gas boundary layer 合灰气体边界层
The structures of shock wave in dusty gas are studied by shock tube experiments.
利用激波管实验对含灰气体激波结构作了研究。
It consists of a dusty, doughnut-shaped cloud of gas and dust that feeds a central supermassive black hole.
它由多尘的环状气体云和不断进入中心巨型黑洞的尘埃组成。
Current theories suggest two ways in which a gaseous, dusty ring around a young star can form into gas-giant planets.
现有的理论提出了两条途径来解释在一个由气体尘埃环围绕的年轻恒星周围如何形成气体巨型行星。
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