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星际A型CH↓3CN-H↓2含超精细能级的碰撞跃迁速率系数的理论计算
曾琴; 裴春传
1995
Source Publication天文学报
ISSN0001-5245
Volume036Issue:001Pages:7
Abstract本文作者利用IOS近似模型,计算了星际分子云条件下A型CH3CN-H2含超精细能级的碰撞跃迁速率系数,温度范围是20K-140K,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/332002/29684
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
曾琴,裴春传. 星际A型CH↓3CN-H↓2含超精细能级的碰撞跃迁速率系数的理论计算[J]. 天文学报,1995,036(001):7.
APA 曾琴,&裴春传.(1995).星际A型CH↓3CN-H↓2含超精细能级的碰撞跃迁速率系数的理论计算.天文学报,036(001),7.
MLA 曾琴,et al."星际A型CH↓3CN-H↓2含超精细能级的碰撞跃迁速率系数的理论计算".天文学报 036.001(1995):7.
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