Effect of Optical Depth on Study of Chemical Properties of Massive Star Forming Clumpsy
文献类型:期刊论文
作者 | Zhou Jianjun![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() ![]() |
刊名 | Chinese Journal of Chemical Physics
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出版日期 | 2020 |
卷号 | 33期号:1页码:114-118 |
关键词 | 恒星形成 团块 分子射电谱线 Stars formation Clumps Molecules Radio lines |
ISSN号 | 1674-0068 |
英文摘要 | Here we present the study on chemical properties of massive star forming clumps using N_2H~+(1-0), H~(13)CO~+(1-0), HCN(1-0) and HN~(13)C(1-0) data from the literature Astron. Astrophys. 563, A97(2014). We found that abundances of H~(13)CO~+ and HN~(13)C are affected by H_2 column densities. As the median values of these two abundances increase by nearly 10 times from stages A to B, H~(13)CO~+ and HN~(13)C are suitable for tracing the evolution of massive star forming clumps. The order of rapidity in growth of abundances of all the four studied molecules from stages A to B, is H~(13)CO~+, HCN, HN~(13)C, and N_2H~+, from the highest to the lowest. Our results suggest that the observing optically thin molecular lines with high angular resolution are necessary to study the chemical evolution of massive star forming clumps. |
语种 | 英语 |
CSCD记录号 | CSCD:6671914 |
源URL | [http://ir.xao.ac.cn/handle/45760611-7/6522] ![]() |
专题 | 研究单元未命名 |
作者单位 | 中国科学院新疆天文台 |
推荐引用方式 GB/T 7714 | Zhou Jianjun,Li Runxia,Quan Donghui,et al. Effect of Optical Depth on Study of Chemical Properties of Massive Star Forming Clumpsy[J]. Chinese Journal of Chemical Physics,2020,33(1):114-118. |
APA | Zhou Jianjun.,Li Runxia.,Quan Donghui.,Esimbek Jarken.,He Yuxin.,...&Zhang Xia.(2020).Effect of Optical Depth on Study of Chemical Properties of Massive Star Forming Clumpsy.Chinese Journal of Chemical Physics,33(1),114-118. |
MLA | Zhou Jianjun,et al."Effect of Optical Depth on Study of Chemical Properties of Massive Star Forming Clumpsy".Chinese Journal of Chemical Physics 33.1(2020):114-118. |
入库方式: OAI收割
来源:新疆天文台
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