科研之友
微信
新浪微博
Facebook
分享链接
摘要
We report on a study of the molecular cloud S64 with observations at millimeter wavelengths of multiple molecular lines of CO isotopes. A weak outflow is found, and its physical parameters are estimated. The departure of the core of S64 from the S64 HIT region indicates that there are still other star formation activities in that region.
- 出版日期2006
- 单位北京大学
