radiationdrivenimplosioninthecepheusbmolecularcloud
文献类型：期刊论文
| 作者 | Sheng Chen; Maohai Huang
|
| 刊名 | researchinastronomyandastrophysics
 |
| 出版日期 | 2010 |
| 卷号 | 000期号:008页码:777 |
| ISSN号 | 1674-4527 |
| 英文摘要 | We analyze large scale mapping observations of the molecular lines in the ^12CO（J= 2-1）,^12CO（J=3-2）,^13CO（J=2-1）,and ^13CO（J=3-2） transition emissions toward the Cepheus B molecular cloud with the KOSMA 3mtelescope. The integrated intensity map of the ^12CO （J = 2 - 1） transition has shown a structure with a compact core and a compact ridge extended to the north-west of the core. The cloud is surrounded by an optically bright rim, where the radiation-driven implosion （RDI） may greatly change the gas properties. The intensities of the CO （J = 3 - 2） transition are higher than those of the CO （J = 2 - 1） transition along the rim area. We find characteristic RDI structure in position-velocity diagrams. Non-LTE large velocity gradient （LVG） model analysis shows that the density and temperature at the edge are higher than that in the center. Our results provide evidences that an RDI is taking place in the Cepheus B molecular cloud. |
| 语种 | 英语 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/39321]  |
| 专题 | 中国科学院国家天文台 |
| 作者单位 | 中国科学院国家天文台 |
| 推荐引用方式 GB/T 7714 | Sheng Chen,Maohai Huang. radiationdrivenimplosioninthecepheusbmolecularcloud[J]. researchinastronomyandastrophysics,2010,000(008):777. |
| APA | Sheng Chen,&Maohai Huang.(2010).radiationdrivenimplosioninthecepheusbmolecularcloud.researchinastronomyandastrophysics,000(008),777. |
| MLA | Sheng Chen,et al."radiationdrivenimplosioninthecepheusbmolecularcloud".researchinastronomyandastrophysics 000.008(2010):777. |
入库方式： OAI收割
来源：国家天文台
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。