会议专题

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

中国天文学会第四届青年天文论坛

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)