PMO OpenIR
星际E型CH↓3CN与H↓2的碰撞跃迁速率系数的理论计算
裴春传; 曾琴
1995
Source Publication天文学报
ISSN0001-5245
Volume036Issue:002Pages:213
Abstract继本文作者对星际A型CH3CN与H2含超精细能级的碰撞过程的研究之后,又计算了星际分子云条件下E型CH3CN与H2的碰撞跃迁速率系数。为研究分子云与恒星形成区的物理、化学性质提供了有用的基础分子数据。
Language英语
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/32089
Collection中国科学院紫金山天文台
Affiliation中国科学院紫金山天文台
First Author Affilication中国科学院紫金山天文台
Recommended Citation
GB/T 7714
裴春传,曾琴. 星际E型CH↓3CN与H↓2的碰撞跃迁速率系数的理论计算[J]. 天文学报,1995,036(002):213.
APA 裴春传,&曾琴.(1995).星际E型CH↓3CN与H↓2的碰撞跃迁速率系数的理论计算.天文学报,036(002),213.
MLA 裴春传,et al."星际E型CH↓3CN与H↓2的碰撞跃迁速率系数的理论计算".天文学报 036.002(1995):213.
Files in This Item:
There are no files associated with this item.
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[裴春传]'s Articles
[曾琴]'s Articles
Baidu academic
Similar articles in Baidu academic
[裴春传]'s Articles
[曾琴]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[裴春传]'s Articles
[曾琴]'s Articles
Terms of Use
No data!
Social Bookmark/Share
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.