CO暗的分子气体中的物理环境
Summary:Determine N、n、T of CO-dark molecular gas on the Galactic plane;Thermal pressures are greater than that of Galactic CNM;Dependence of temperature results in large uncertainty of dark molecular fraction in low temperature range;Maybe the first time to find young,transitional molecular clouds without CO formations,Other emission lines like OH、CH、HCO+ are necessary to convince this。
一氧化碳 分子气体 物理环境
汤宁宇 李菂
国内会议
南京
中文
1-27
2015-07-01(万方平台首次上网日期,不代表论文的发表时间)