The Correlation Between Dust and Gas Contents in Molecular Clouds
文献类型:期刊论文
作者 | Li RZ(李睿智)2,3,4![]() ![]() |
刊名 | ASTRONOMICAL JOURNAL
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出版日期 | 2024-11-01 |
卷号 | 168期号:5 |
ISSN号 | 0004-6256 |
DOI | 10.3847/1538-3881/ad77a3 |
产权排序 | 第1完成单位 |
文献子类 | Article |
英文摘要 | Molecular clouds are regions of dense gas and dust in space where new stars and planets are born. There is a strong correlation between the distribution of dust and molecular gas in molecular clouds. The present work focuses on the three-dimensional morphological comparisons between dust and gas in 567 molecular clouds identified in a previously published catalog. We confirm a sample of 112 molecular clouds, where the cloud morphology based on CO observations and dust observations displays good overall consistency. There are up to 334 molecular clouds whose dust distribution might be related to the distribution of gas. We are unable to find gas structures that correlate with the shape of the dust distribution in 24 molecular clouds. For the 112 molecular clouds where the dust distribution correlates very well with the distribution of gas, we use CO observational data to measure the physical properties of these molecular clouds and compare them with the results derived from dust, exploring the correlation between gas and dust in the molecular clouds. We found that the gas and dust in the molecular clouds have a fairly good linear relationship, with a gas-to-dust ratio of GDR=(2.80-0.34+0.37)x1021cm-2mag-1 . The ratio varies considerably among different molecular clouds. We measured the scale height of dust-CO clouds exhibiting strong correlations, finding hZ=43.3-3.5+4.0 pc. |
学科主题 | 天文学 ; 星系与宇宙学 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
WOS关键词 | CO-DARK GAS ; LARGE CATALOG ; MILKY-WAY ; ACCURATE DISTANCES ; INTERSTELLAR DUST ; CONVERSION FACTOR ; SOLAR NEIGHBORHOOD ; FORMATION HISTORY ; BILLION STARS ; H-I |
资助项目 | Yunnan University (YNU)https://doi.org/10.13039/501100007839[2019YFA0405500]; National Key R&D Program of China[12173034]; National Key R&D Program of China[12322304]; National Natural Science Foundation of China[202010673028]; Innovation and Entrepreneurship Training Projects for College Student of Yunnan University[C619300A034]; Yunnan University[CMS-CSST-2021-A09]; Yunnan University[CMS-CSST-2021-A08]; Yunnan University[CMS-CSST-2021-B03]; China Manned Space Project |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:001341348600001 |
出版者 | IOP Publishing Ltd |
资助机构 | Yunnan University (YNU)https://doi.org/10.13039/501100007839[2019YFA0405500] ; National Key R&D Program of China[12173034, 12322304] ; National Natural Science Foundation of China[202010673028] ; Innovation and Entrepreneurship Training Projects for College Student of Yunnan University[C619300A034] ; Yunnan University[CMS-CSST-2021-A09, CMS-CSST-2021-A08, CMS-CSST-2021-B03] ; China Manned Space Project |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/27662] ![]() |
专题 | 星系类星体研究组 |
作者单位 | 1.South-Western Institute for Astronomy Research, Yunnan University, Kunming 650504, People's Republic of China; bchen@ynu.edu.cn, gxli@ynu.edu.cn 2.Department of Astronomy, Yunnan University, Kunming 650504, People's Republic of China; 3.University of Chinese Academy of Sciences, Beijing 101408, People's Republic of China; 4.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People's Republic of China; |
推荐引用方式 GB/T 7714 | Li RZ,Chen, Bing-Qiu,Li, Guang-Xing,et al. The Correlation Between Dust and Gas Contents in Molecular Clouds[J]. ASTRONOMICAL JOURNAL,2024,168(5). |
APA | 李睿智,Chen, Bing-Qiu,Li, Guang-Xing,王柏廷,Ren, Hao-Ming,&Guo, Qi-Ning.(2024).The Correlation Between Dust and Gas Contents in Molecular Clouds.ASTRONOMICAL JOURNAL,168(5). |
MLA | 李睿智,et al."The Correlation Between Dust and Gas Contents in Molecular Clouds".ASTRONOMICAL JOURNAL 168.5(2024). |
入库方式: OAI收割
来源:云南天文台
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