PMO OpenIR
The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17
Liu, Tie1,2; Kim, Kee-Tae1; Juvela, Mika3; Wang, Ke4; Tatematsu, Ken'ichi5; Di Francesco, James6,7; Liu, Sheng-Yuan8; Wu, Yuefang9; Thompson, Mark10; Fuller, Gary11; Eden, David12; Li, Di13,14; Ristorcelli, I.15; Kang, Sung-ju1; Lin, Yuxin16; Johnstone, D.6,7; He, J. H.17,18,19; Koch, P. M.8; Sanhueza, Patricio5; Qin, Sheng-Li20,21; Zhang, Q.22; Hirano, N.8; Goldsmith, Paul F.23; Evans, Neal J., II1,24; White, Glenn J.25,26; Choi, Minho1; Lee, Chang Won1,27; Toth, L. V.28,29; Mairs, Steve6; Yi, H. -W.30; Tang, Mengyao20,21; Soam, Archana1; Peretto, N.31; Samal, Manash R.32; Fich, Michel33; Parsons, Harriet2; Yuan, Jinghua13; Zhang, Chuan-Peng13; Malinen, Johanna34; Bendo, George J.11; Rivera-Ingraham, A.35; Liu, Hong-Li36,37,38; Wouterloot, Jan2; Li, Pak Shing39; Qian, Lei13; Rawlings, Jonathan40; Rawlings, Mark G.2; Feng, Siyi41; Aikawa, Yuri42; Akhter, S.43; Alina, Dana44; Bell, Graham2; Bernard, J. -P.15; Blain, Andrew45; Bogner, Rebeka28; Bronfman, L.19; Byun, D. -Y.1; Chapman, Scott46; Chen, Huei-Ru47,48; Chen, M.6; Chen, Wen-Ping32; Chen, X.49; Chen, Xuepeng50; Chrysostomou, A.10; Cosentino, Giuliana40; Cunningham, M. R.43; Demyk, K.15; Drabek-Maunder, Emily51; Doi, Yasuo52; Eswaraiah, C.47,48; Falgarone, Edith53; Feher, O.28,54; Fraser, Helen25; Friberg, Per2,3; Garay, G.19; Ge, J. X.17; Gear, W. K.31; Greaves, Jane31; Guan, X.55; Harvey-Smith, Lisa43,56; Hasegawa, Tetsuo5; Hatchell, J.57; He, Yuxin58; Henkel, C.16,59; Hirota, T.5; Holland, W.60,61; Hughes, A.15; Jarken, E.58; Ji, Tae-Geun30; Jimenez-Serra, Izaskun62; Kang, Miju1; Kawabata, Koji S.63,64; Kim, Gwanjeong5; Kim, Jungha30; Kim, Jongsoo1; Kim, Shinyoung1; Koo, B. -C.65; Kwon, Woojin1,66; Kuan, Yi-Jehng67; Lacaille, K. M.46,68; Lai, Shih-Ping8,47,48; Lee, C. F.8; Lee, J. -E.30; Lee, Y. -U.1; Li, Dalei58; Li, Hua-Bai69; Lo, N.19; Lopez, John A. P.43; Lu, Xing5; Lyo, A-Ran1; Mardones, D.19; Marston, A.70; McGehee, P.71; Meng, F.55; Montier, L.15; Montillaud, Julien72; Moore, T.12; Morata, O.8; Moriarty-Schieven, Gerald H.6; Ohashi, S.5; Pak, Soojong30; Park, Geumsook1; Paladini, R.71; Pattle, Kate M.73; Pech, Gerardo8; Pelkonen, V. -M.72; Qiu, K.74; Ren, Zhi-Yuan13; Richer, John75; Saito, M.5; Sakai, Takeshi76; Shang, H.8; Shinnaga, Hiroko77; Stamatellos, Dimitris73; Tang, Y. -W.8; Traficante, Alessio78; Vastel, Charlotte15; Viti, S.40; Walsh, Andrew79; Wang, Bingru13; Wang, Hongchi50; Wang, Junzhi49; Ward-Thompson, D.73; Whitworth, Anthony31; Xu, Ye50; Yang, J.50; Yang, Yao-Lun80; Yuan, Lixia13; Zavagno, A.81; Zhang, Guoyin13; Zhang, H. -W.9; Zhou, Chenlin50; Zhou, Jianjun58; Zhu, Lei13; Zuo, Pei13; Zhang, Chao2
2018-02-01
Source PublicationASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
ISSN0067-0049
Volume234Issue:2Pages:31
Corresponding AuthorLiu, Tie(liutiepku@gmail.com)
AbstractThe low dust temperatures (< 14 K) of Planck Galactic cold clumps (PGCCs) make them ideal targets to probe the initial conditions and very early phase of star formation. "TOP-SCOPE" is a joint survey program targeting similar to 2000 PGCCs in J = 1-0 transitions of CO isotopologues and similar to 1000 PGCCs in 850 mu m continuum emission. The objective of the "TOP-SCOPE" survey and the joint surveys (SMT 10 m, KVN 21 m, and NRO 45 m) is to statistically study the initial conditions occurring during star formation and the evolution of molecular clouds, across a wide range of environments. The observations, data analysis, and example science cases for these surveys are introduced with an exemplar source, PGCC G26.53+0.17 (G26), which is a filamentary infrared dark cloud (IRDC). The total mass, length, and mean line mass (M/L) of the G26 filament are similar to 6200 M-circle dot, similar to 12 pc, and similar to 500 M-circle dot pc(-1), respectively. Ten massive clumps, including eight starless ones, are found along the filament. The most massive clump as a whole may still be in global collapse, while its denser part seems to be undergoing expansion owing to outflow feedback. The fragmentation in the G26 filament from cloud scale to clump scale is in agreement with gravitational fragmentation of an isothermal, nonmagnetized, and turbulent supported cylinder. A bimodal behavior in dust emissivity spectral index (beta) distribution is found in G26, suggesting grain growth along the filament. The G26 filament may be formed owing to large-scale compression flows evidenced by the temperature and velocity gradients across its natal cloud.
KeywordISM: abundances ISM: clouds ISM: kinematics and dynamics stars: formation surveys
DOI10.3847/1538-4365/aaa3dd
WOS KeywordINFRARED DARK CLOUD ; FILAMENTARY MOLECULAR CLOUDS ; CLERK MAXWELL TELESCOPE ; STAR-FORMATION ; INITIAL CONDITIONS ; LINE-PROFILES ; LARGE-SCALE ; GOULD BELT ; DENSE GAS ; FRAGMENTATION
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000424013500005
PublisherIOP PUBLISHING LTD
Citation statistics
Cited Times:18[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/22215
Collection中国科学院紫金山天文台
Corresponding AuthorLiu, Tie
Affiliation1.Korea Astron & Space Sci Inst, 776 Daedeokdaero, Daejeon 34055, South Korea
2.East Asian Observ, 660 N Aohoku Pl, Hilo, HI 96720 USA
3.Univ Helsinki, Dept Phys, POB 64, FI-00014 Helsinki, Finland
4.European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany
5.Natl Inst Nat Sci, Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
6.NRC Herzberg Astron & Astrophys, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada
7.Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 1A1, Canada
8.Acad Sinica, Inst Astron & Astrophys, 11F Astron Math Building,AS-NTU 1,Sect 4, Taipei 10617, Taiwan
9.Peking Univ, Dept Astron, Beijing 100871, Peoples R China
10.Univ Hertfordshire, Sch Phys Astron & Math, Ctr Astrophys Res, Coll Lane, Hatfield AL10 9AB, Herts, England
11.Univ Manchester, Sch Phys & Astron, UK ALMA Reg Ctr Node, Jodrell Bank Ctr Astrophys, Oxford Rd, Oxford M13 9PL, England
12.Liverpool John Moores Univ, Astrophys Res Inst, IC2,Liverpool Sci Pk,146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England
13.Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China
14.Chinese Acad Sci, Key Lab Radio Astron, Nanjing 210008, Jiangsu, Peoples R China
15.Univ Toulouse, CNRS, IRAP, UPS,CNES, Toulouse, France
16.Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany
17.Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Yunnan Observ, POB 110, Kunming 650011, Yunnan, Peoples R China
18.CASSACA, Camino El Observ 1515, Santiago, Chile
19.Univ Chile, Dept Astron, Santiago, Chile
20.Yunnan Univ, Dept Astron, Kunming 650091, Yunnan, Peoples R China
21.Yunnan Univ, Key Lab Astroparticle Phys Yunnan Prov, Kunming 650091, Yunnan, Peoples R China
22.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
23.CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
24.Univ Texas Austin, Dept Astron, 2515 Speedway,Stop C1400, Austin, TX 78712 USA
25.Open Univ, Dept Phys & Astron, Walton Hall, Milton Keynes MK7 6AA, Bucks, England
26.STFC Rutherford Appleton Lab, RAL Space, Chilton OX11 0QX, England
27.Univ Sci & Technol, 176 Gajeong Dong, Daejeon, South Korea
28.Eotvos Lorand Univ, Dept Astron, Pazmany Peter Setany 1-A, H-1117 Budapest, Hungary
29.Hungarian Acad Sci, Konkoly Observ, Konkoly Thege Miklosut 15-17, H-1121 Budapest, Hungary
30.Kyung Hee Univ, Sch Space Res, Yongin 17104, Gyeonggi Do, South Korea
31.Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales
32.Natl Cent Univ, Inst Astron, Jhongli 32001, Taiwan
33.Univ Waterloo, Dept Phys & Astron, Waterloo, ON N2L 3G1, Canada
34.Univ Cologne, Inst Phys 1, Zulpicher Str 77, D-50937 Cologne, Germany
35.European Space Astron Ctr ESA ESAC, Operat Dept, Madrid, Spain
36.Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China
37.Univ Concepcion, Dept Astron, Av Esteban Iturra S-N,Dist Univ,160-C, Concepcion, Chile
38.Chinese Acad Sci, South Amer Ctr Astron, Beijing, Peoples R China
39.Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
40.UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England
41.Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany
42.Univ Tsukuba, Ctr Computat Sci, 1-1-1 Tennodai, Tsukuba, Ibaraki 3058577, Japan
43.Univ New South Wales, Sch Phys, Sydney, NSW 2052, Australia
44.Nazarbayev Univ, Sch Sci & Technol, Dept Phys, Astana 010000, Kazakhstan
45.Univ Leicester, Phys & Astron, 1 Univ Rd, Leicester LE1 7RH, Leics, England
46.Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS B3H 4R2, Canada
47.Natl Tsing Hua Univ, Inst Astron, Hsinchu, Taiwan
48.Natl Tsing Hua Univ, Dept Phys, Hsinchu, Taiwan
49.Chinese Acad Sci, Shanghai Astron Observ, Key Lab Res Galaxies & Cosmol, 80 Nandan Rd, Shanghai 200030, Peoples R China
50.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
51.Imperial Coll London, Blackett Lab, Prince Consort Rd, London SW7 2BB, England
52.Univ Tokyo, Grad Sch Arts & Sci, Dept Earth Sci & Astron, 3-8-1 Komaba, Tokyo 1538902, Japan
53.Univ Paris 06, UPMC, Sorbonne Univ, CNRS,PSL Res Univ,Observ Paris,LERMA,Ecole Normal, F-75005 Paris, France
54.Hungarian Acad Sci, Res Ctr Astron & Earth Sci, Konkoly Observ, Konkoly Thege Miklos Ut 15-17, H-1121 Budapest, Hungary
55.Univ Cologne, Phys Inst, Zulpicher Str 77, D-50937 Cologne, Germany
56.CSIRO Astron & Space Sci, POB 76, Epping, NSW, Australia
57.Univ Exeter, Phys & Astron, Stocker Rd, Exeter EX4 4QL, Devon, England
58.Univ Chinese Acad Sci, Chinese Acad Sci, Xinjiang Astron Observ, Beijing, Peoples R China
59.Abdulaziz Univ, Astron Dept, POB 80203, Jeddah 21589, Saudi Arabia
60.UK Astron Technol Ctr, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
61.Univ Edinburgh, Inst Astron, Royal Observ, Blackford Hill, Edinburgh EH9 3HJ, Midlothian, Scotland
62.Queen Mary Univ London, Sch Phys & Astron, Mile End Rd, London E1 4NS, England
63.Hiroshima Univ, Hiroshima Astrophys Sci Ctr, Higashihiroshima, Hiroshima 7398526, Japan
64.Hiroshima Univ, Dept Phys Sci, Higashihiroshima 7398526, Japan
65.Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea
66.Korea Univ Sci & Technol, 217 Gajeong Ro, Daejeon 34113, South Korea
67.Natl Taiwan Normal Univ, Dept Earth Sci, 88 Sect 4,Ting Chou Rd, Taipei 116, Taiwan
68.McMaster Univ, Dept Phys & Astron, Hamilton, ON L8S 4M1, Canada
69.Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China
70.ESA STScI, 3700 San Martin Dr, Baltimore, MD 21218 USA
71.CALTECH, Infrared Proc Anal Ctr, 770 South Wilson Ave, Pasadena, CA 91125 USA
72.Univ Bourgogne Franche Comte, CNRS, UMR 6213, Inst UTINAM, Franche Comte, France
73.Univ Cent Lancashire, Jeremiah Horrocks Inst Math Phys & Astron, Preston PR1 2HE, Lancs, England
74.Nanjing Univ, Sch Astron & Space Sci, Nanjing 210023, Jiangsu, Peoples R China
75.Cavendish Lab, Astrophys Grp, JJ Thomson Ave, Cambridge CB3 0HE, England
76.Univ Electrocommun, Grad Sch Informat & Engn, Chofu, Tokyo 1828585, Japan
77.Kagoshima Univ, Grad Sch Sci & Engn, Dept Phys & Astron, 1-21-35 Korimoto, Kagoshima 8900065, Japan
78.IAPS INAF, Via Fosso Cavaliere 100, Rome, Italy
79.Curtin Univ, Int Ctr Radio Astron Res, GPO Box U1987, Perth, WA 6845, Australia
80.Univ Texas Austin, Dept Astron, 2515 Speedway,Stop C1400, Austin, TX 78712 USA
81.Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France
Recommended Citation
GB/T 7714
Liu, Tie,Kim, Kee-Tae,Juvela, Mika,et al. The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17[J]. ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,2018,234(2):31.
APA Liu, Tie.,Kim, Kee-Tae.,Juvela, Mika.,Wang, Ke.,Tatematsu, Ken'ichi.,...&Zhang, Chao.(2018).The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17.ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES,234(2),31.
MLA Liu, Tie,et al."The TOP-SCOPE Survey of Planck Galactic Cold Clumps: Survey Overview and Results of an Exemplar Source, PGCC G26.53+0.17".ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES 234.2(2018):31.
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