中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
热门
A Systematic TMRT Observational Study of Galactic C-12/C-13 Ratios from Formaldehyde

文献类型:期刊论文

作者Jian, J. M.7; Huang, J.7; Li, Y. Q.7; Wang, Y. X.7; Zeng, Z. A.7; Li, J.1,4; Wu, Y. J.1,4; Tang, X. D.1,2,6; Jia, L. W.7; Mufakharov, T.3,4
刊名ASTROPHYSICAL JOURNAL
出版日期2019-06-01
卷号877期号:2页码:15
ISSN号0004-637X
关键词Galaxy: evolution HII regions ISM: abundances
DOI10.3847/1538-4357/ab17d6
通讯作者Zhang, J. S.(jszhang@gzhu.edu.cn)
英文摘要We present observations of the C-band 1(10)-1(11) (4.8 GHz) and Ku-band 2(11)-2(12) (14.5 GHz) K-doublet lines of H2CO and the C-band 1(10)-1(11) (4.6 GHz) line of (H2CO)-C-13 toward a large sample of Galactic molecular clouds, through the Shanghai Tianma 65 m radio telescope (TMRT). Our sample with 112 sources includes strong H2CO sources from the TMRT molecular line survey at C-band and other known H2CO sources. All three lines are detected toward 38 objects (43 radial velocity components) yielding a detection rate of 34%. Complementary observations of their continuum emission at both C- and Ku-bands were performed. Combining spectral line parameters and continuum data, we calculate the column densities, the optical depths and the isotope ratio (H2CO)-C-12/(H2CO)-C-13 for each source. To evaluate photon trapping caused by sometimes significant opacities in the main isotopologue's rotational mm-wave lines connecting our measured K-doublets, and to obtain C-12/C-13 abundance ratios, we used the RADEX non-LIE model accounting for radiative transfer effects. This implied the use of the new collision rates from Wiesenfeld & Faure. Also implementing distance values from trigonometric parallax measurements for our sources, we obtain a linear fit of C-12/C-13 = (5.08 +/- 1.10)D-GC + (11.86 +/- 6.60), with a con elation coefficient of 0.58. D-GC refers to Galactocentric distances. Our C-12/C-13 C ratios agree very well with the ones deduced from CN and (CO)-O-1-O-8 but are lower than those previously reported on the basis of H2CO, tending to suggest that the bulk of the H2CO in our sources was formed on dust grain mantles and not in the gas phase.
WOS关键词STAR-FORMATION REGIONS ; MOLECULAR CLOUDS ; DISTANCE AMBIGUITIES ; DENSE GAS ; H2CO ; ISOTOPE ; C-13 ; GALAXY ; ABUNDANCES ; EXCITATION
资助项目Natural Science Foundation of China[11473007] ; Natural Science Foundation of China[11590782] ; Guangzhou Education Bureau[1201410593]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000470807700015
资助机构Natural Science Foundation of China ; Guangzhou Education Bureau
源URL[http://ir.xao.ac.cn/handle/45760611-7/2774]  
专题恒星形成与演化研究团组
通讯作者Zhang, J. S.
作者单位1.Chinese Acad Sci, Key Lab Radio Astron, Beijing, Peoples R China
2.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
3.Kazan Fed Univ, 18 Kremlyovskaya St, Kazan 420008, Russia
4.Chinese Acad Sci, Shanghai Astron Observ, Shanghai 200030, Peoples R China
5.King Abdulaziz Univ, Astron Dept, POB 80203, Jeddah 21589, Saudi Arabia
6.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
7.Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Guangdong, Peoples R China
推荐引用方式
GB/T 7714
Jian, J. M.,Huang, J.,Li, Y. Q.,et al. A Systematic TMRT Observational Study of Galactic C-12/C-13 Ratios from Formaldehyde[J]. ASTROPHYSICAL JOURNAL,2019,877(2):15.
APA Jian, J. M..,Huang, J..,Li, Y. Q..,Wang, Y. X..,Zeng, Z. A..,...&Yan, Y. T..(2019).A Systematic TMRT Observational Study of Galactic C-12/C-13 Ratios from Formaldehyde.ASTROPHYSICAL JOURNAL,877(2),15.
MLA Jian, J. M.,et al."A Systematic TMRT Observational Study of Galactic C-12/C-13 Ratios from Formaldehyde".ASTROPHYSICAL JOURNAL 877.2(2019):15.

入库方式: OAI收割

来源:新疆天文台

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。