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Chemically Fresh Gas Inflows Detected in a Nearby High-mass Star-forming Region
Chen, Xi1,2; Ren, Zhi-Yuan3; Li, Da-Lei4; Liu, Tie2; Wang, Ke5; Shen, Zhi-Qiang2; Ellingsen, Simon P.6; Sobolev, Andrej M.7; Mei, Ying1; Li, Jing-Jing8; Wu, Yue-Fang5; Kim, Kee-Tae9,10
2021-12-01
Source PublicationASTROPHYSICAL JOURNAL LETTERS
ISSN2041-8205
Volume923Issue:1Pages:20
Contribution Rank4
AbstractWe report the detection of a chemically fresh inflow that is feeding high-mass young-stellar-object (HMYSO) growth in the nearby high-mass star-forming region G352.63 made with both the Atacama Large Millimeter/submillimeter Array (ALMA) and the Submillimeter Array (SMA). High-quality images of the dust and molecular lines from both ALMA and SMA have consistently revealed a gravitationally controlled cold (similar to 10 K) gas inflow of chemically fresh molecules (e.g., CCH and HC3N) toward the central HMYSO and its surrounding dense gas structure, which has a possible torus- or disk-like morphology. The HMYSO is also observed to have an outflow, which is nearly perpendicular to the torus and its parental filament, and thus can be clearly separated from the inflows. These kinematic features provide observational evidence to support the conjecture that the infalling streamers in high-mass star-forming regions could proceed in a similar process to that observed in low-mass counterparts. The chemically fresh infalling streamers could also be involved in the disk or torus configuration, fragmentation, and accretion bursts that occur in both simulations and observations.
DOI10.3847/2041-8213/ac3ec8
Indexed BySCI
Language英语
WOS KeywordMOLECULAR CLOUDS ; DARK CLOUDS ; DENSE CORES ; ACCRETION ; PROTOSTARS ; TURBULENT ; FILAMENTS ; DISC
Funding ProjectNational Natural Science Foundation of China[11873002] ; National Natural Science Foundation of China[12011530065] ; National Natural Science Foundation of China[11590781] ; Guangdong Province Universities and Colleges Pearl River Scholar Funded Scheme (2019) ; ARC Discovery Project[DP180101061] ; Ministry of Education and Science of the Russian Federation[FEUZ-2020-0030]
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000730635800001
PublisherIOP Publishing Ltd
Funding OrganizationNational Natural Science Foundation of China ; Guangdong Province Universities and Colleges Pearl River Scholar Funded Scheme (2019) ; ARC Discovery Project ; Ministry of Education and Science of the Russian Federation
Citation statistics
Cited Times:6[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://ir.xao.ac.cn/handle/45760611-7/4405
Collection射电天文研究室_恒星形成与演化研究团组
Corresponding AuthorChen, Xi; Ren, Zhi-Yuan
Affiliation1.Guangzhou Univ, Ctr Astrophys, Guangzhou 510006, Peoples R China
2.Chinese Acad Sci, Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
3.Chinese Acad Sci, Natl Astron Observ, Datun Rd A20, Beijing, Peoples R China
4.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
5.Peking Univ, Kavli Inst Astron & Astrophys, 5 Yiheyuan Rd, Beijing 100871, Peoples R China
6.Univ Tasmania, Sch Nat Sci, Private Bag 37, Hobart, Tas 7001, Australia
7.Ural Fed Univ, 19 Mira St, Ekaterinburg 620002, Russia
8.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China
9.Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea
10.Univ Sci & Technol Korea UST, 217 Gajeong Ro, Daejeon 34113, South Korea
Recommended Citation
GB/T 7714
Chen, Xi,Ren, Zhi-Yuan,Li, Da-Lei,et al. Chemically Fresh Gas Inflows Detected in a Nearby High-mass Star-forming Region[J]. ASTROPHYSICAL JOURNAL LETTERS,2021,923(1):20.
APA Chen, Xi.,Ren, Zhi-Yuan.,Li, Da-Lei.,Liu, Tie.,Wang, Ke.,...&Kim, Kee-Tae.(2021).Chemically Fresh Gas Inflows Detected in a Nearby High-mass Star-forming Region.ASTROPHYSICAL JOURNAL LETTERS,923(1),20.
MLA Chen, Xi,et al."Chemically Fresh Gas Inflows Detected in a Nearby High-mass Star-forming Region".ASTROPHYSICAL JOURNAL LETTERS 923.1(2021):20.
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