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MCELS (Magellanic Cloud Emission-line Survey) : ウィキペディア英語版 | MCELS (Magellanic Cloud Emission-line Survey)
The Magellanic Cloud Emission Line Survey (MCELS) is a joint project of Cerro Tololo Inter-American Observatory (Chile) and the University of Michigan using the CTIO Curtis/Schmidt Telescope. The main goal of the project is to trace the ionized gas in the Magellanic Clouds using narrow-band filters ((II ), Hα and (III )). Those emission lines are produced by different astrophysical objects and processes. == Scientific Motivation == To investigate the physical properties of the interstellar medium of these galaxies.
抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)』 ■ウィキペディアで「MCELS (Magellanic Cloud Emission-line Survey)」の詳細全文を読む
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