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L183, a quiescent core?
Zhou, JJ1,2; Zheng, XW1; Chen, YX1
2001-06-01
Source PublicationCHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS
Volume1Issue:3Pages:250-256
Contribution Rank1
AbstractSome observed results of NH3 (1, 1) and (2,2) line emission in the starless dark cloud L183 are reported. Our observation suggests that the dense core of L183 has a size of similar to 0.16pc x0.1pc with a mass of similar to 12M(circle dot). A velocity gradient of 4km s(-1)pc(-1) from the north to the south was detected. The velocity shift corresponds to a central mass of similar to 5M(circle dot). If it is caused by rotation, the mass would be much less than the value above. This suggests that there may be more mass in the envelope of L183 than in the central region. The analysis of our data and the evidence in the literature about L183 indicate that it may be undergoing a process of collapsing to form a low-mass binary dense core.
KeywordIsm : Clouds Stars : Formation Stars : Low-mass
SubtypeArticle
WOS HeadingsScience & Technology ; Physical Sciences
Indexed BySCI
Language英语
WOS KeywordL134N MOLECULAR CORE ; DENSE CORES ; PROTOSTELLAR COLLAPSE ; DARK CLOUDS
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000172248900007
Citation statistics
Cited Times:1[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/854
Collection射电天文研究室_恒星形成与演化研究团组
射电天文研究室
Corresponding AuthorZheng, XW
Affiliation1.Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China
2.Chinese Acad Sci, Urumqi Astron Observ, Xingjiang 830011, Peoples R China
First Author AffilicationXinjiang Astronomical Observatory, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
Zhou, JJ,Zheng, XW,Chen, YX. L183, a quiescent core?[J]. CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,2001,1(3):250-256.
APA Zhou, JJ,Zheng, XW,&Chen, YX.(2001).L183, a quiescent core?.CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS,1(3),250-256.
MLA Zhou, JJ,et al."L183, a quiescent core?".CHINESE JOURNAL OF ASTRONOMY AND ASTROPHYSICS 1.3(2001):250-256.
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