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Three-dimensional Projection Effects on Chemistry in a Planck Galactic Cold Clump
Ge, J. X.1; Mardones, Diego1,2; He JH(何金华)1,3,4; Rawlings, Jonathan M. C.5; Liu, Sheng-Yuan6; Lee, Jeong-Eun7; Tatematsu, Ken'ichi8,9; Liu, Tie10,11; Zhu, Lei4; Chang, Qiang12; Inostroza, Natalia13; Feng, S.8,14,15
发表期刊ASTROPHYSICAL JOURNAL
2020-03-01
卷号891期号:1页码:13
DOI10.3847/1538-4357/ab7007
产权排序第3完成单位
收录类别SCI
关键词Astrochemistry Dense interstellar clouds Interstellar abundances Chemical abundances
摘要

Offsets of molecular line emission peaks from continuum peaks are very common but frequently difficult to explain with a single spherical cloud chemical model. We propose that the spatial projection effects of an irregular three-dimensional (3D) cloud structure can be a solution. This work shows that the idea can be successfully applied to the Planck cold clump G224.4-0.6 by approximating it with four individual spherically symmetric cloud cores whose chemical patterns overlap with each other to produce observable line maps. With the empirical physical structures inferred from the observation data of this clump and a gas-grain chemical model, the four cores can satisfactorily reproduce its 850 mu m continuum map and the diverse peak offsets of CCS, HC3N, and N2H+ simultaneously at chemical ages of about 8 x 10(5) similar to 3 x 10(6) yr. The 3D projection effects on chemistry has the potential to explain such asymmetrical distributions of chemicals in many other molecular clouds.

资助项目FONDECYT[3170768] ; "Light of West China" program of the Chinese Academy of Sciences (CAS) ; CONICYT[Basal AFB-170002] ; National Natural Science Foundation of China[11873086] ; National Natural Science Foundation of China[U1631237] ; Yunnan Province of China[2017HC018] ; National Research Foundation of Korea[NRF-2018R1A2B6003423] ; Korea Astronomy and Space Science Institute ; CONICYT International Networks for young researchers[REDI170243] ; CONICYT International Networks for young researchers[CONICYT/PCI/REDI170243] ; CONICYT International Networks for young researchers[REDES190113] ; EACOA fellowship from the East Asia Core Observatories Association ; Chinese Academy of Sciences (CAS)
项目资助者FONDECYT[3170768] ; "Light of West China" program of the Chinese Academy of Sciences (CAS) ; CONICYT[Basal AFB-170002] ; National Natural Science Foundation of China[11873086, U1631237] ; Yunnan Province of China[2017HC018] ; National Research Foundation of Korea[NRF-2018R1A2B6003423] ; Korea Astronomy and Space Science Institute ; CONICYT International Networks for young researchers[REDI170243, CONICYT/PCI/REDI170243, REDES190113] ; EACOA fellowship from the East Asia Core Observatories Association ; Chinese Academy of Sciences (CAS)
语种英语
学科领域天文学 ; 恒星与银河系
文章类型Article
出版者IOP PUBLISHING LTD
出版地TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN0004-637X
URL查看原文
WOS记录号WOS:000518952200001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]STARLESS CORE ; DENSE CORES ; DARK CLOUDS ; DEPLETION ; EVOLUTION ; MODELS ; N2H+
引用统计
被引频次:6[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/22531
专题大样本恒星演化研究组
通讯作者Ge, J. X.
作者单位1.Departamento de Astronomía, Universidad de Chile, Camino el Observatorio 1515, Las Condes, Santiago, Chile
2.Centre for Astrochemical Studies, Max-Planck-Institute for Extraterrestrial Physics, Giessenbachstrasse 1, D-85748, Garching, Germany
3.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, People's Republic of China
4.Chinese Academy of Sciences South America Center for Astronomy, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People's Republic of China
5.Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK
6.Institute of Astronomy and Astrophysics, Academia Sinica. 11F of Astronomy-Mathematics Building, AS/NTU No. 1, Section 4, Roosevelt Rd., Taipei 10617, Taiwan
7.School of Space Research, Kyung Hee University, Yongin-si, Republic of Korea
8.National Astronomical Observatory of Japan, National Institutes of Natural Sciences, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
9.Department of Astronomical Science, SOKENDAI (The Graduate University for Advanced Studies), 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan
10.Shanghai Astronomical Observatory, Chinese Academy of Sciences, 80 Nandan Road, Shanghai 200030, People's Republic of China
11.East Asian Observatory, 660 N. A'ohoku Place, Hilo, HI 96720, USA
12.School of Physics and Optoelectronic Engineering, Shandong University of Technology, Zibo 255000, People's Republic of China
13.Universidad Autónoma de Chile, Facultad de Ingeniería, Núcleo de Astroquímica & Astrofísica, Av. Pedro de Valdivia 425, Providencia, Santiago, Chile
14.National Astronomical Observatory of China, Datun Road 20, Chaoyang, Beijing, 100012, People's Republic of China
15.CAS Key Laboratory of FAST, NAOC, Chinese Academy of Sciences, People's Republic of China
推荐引用方式
GB/T 7714
Ge, J. X.,Mardones, Diego,He JH,et al. Three-dimensional Projection Effects on Chemistry in a Planck Galactic Cold Clump[J]. ASTROPHYSICAL JOURNAL,2020,891(1):13.
APA Ge, J. X..,Mardones, Diego.,He JH.,Rawlings, Jonathan M. C..,Liu, Sheng-Yuan.,...&Feng, S..(2020).Three-dimensional Projection Effects on Chemistry in a Planck Galactic Cold Clump.ASTROPHYSICAL JOURNAL,891(1),13.
MLA Ge, J. X.,et al."Three-dimensional Projection Effects on Chemistry in a Planck Galactic Cold Clump".ASTROPHYSICAL JOURNAL 891.1(2020):13.
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