CO LF and molecular gas mass density
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Cold molecular gas, largely traced by CO emission, is the primary fuel for star formation, making it essential for understanding galaxy evolution. ALMA has made significant...
冷分子气体主要通过一氧化碳(CO)辐射进行示踪,是恒星形成的核心燃料,因此对于理解星系演化至关重要。阿塔卡马大型毫米/亚毫米波阵列(Atacama Large Millimeter/submillimeter Array,ALMA)已取得了显著的……



