【摘 要】
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We investigate gas and dust physical properties and chemistry of diffuse interstellar medium in the Large Magellanic Cloud (LMC).Most of the interstellar gas inhabit in photo dissociation regions (PDR
【出 处】
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9th East Asian Meeting on Astronomy(东亚天文会议)
论文部分内容阅读
We investigate gas and dust physical properties and chemistry of diffuse interstellar medium in the Large Magellanic Cloud (LMC).Most of the interstellar gas inhabit in photo dissociation regions (PDR) in galaxies,where FUV radiation from hot stars creates a layered structure.This includes,a layer of predominantly neutral gas residing outside HII regions and a layer of HI/C+/Si+,H2,and neutral oxygen.
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