中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
CHIMPS2: 13CO J=3→2 emission in the central molecular zone

文献类型:期刊论文

作者King, S. M.5; Moore, T. J. T.5; Henshaw, J. D.5; Longmore, S. N.5; Eden, D. J.4; Rigby, A. J.3; Rosolowsky, E.2; Tahani, K.13; Su, Y.1,12; Yiping, A.1,12
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2024-08-07
卷号533期号:1页码:131-142
关键词stars: formation ISM: molecules ISM: structure Galaxy: centre submillimetre: ISM
ISSN号0035-8711
DOI10.1093/mnras/stae1854
产权排序7
英文摘要We present the initial data for the (J = 3 -> 2) transition of (CO)-C-13 obtained from the central molecular zone (CMZ) of the Milky Way as part of the CO Heterodyne Inner Milky Way Plane Survey 2 (CHIMPS2). Covering 359 degrees <= l <= 1 degrees and |b| <= 0.5 degrees with an angular resolution of 19 arcsec, velocity resolution of 1 km s(-1), and rms Delta T-A(& lowast;) = 0.59K at these resolutions, our observations unveil the complex structure of the CMZ molecular gas in improved detail. Complemented by the (CO)-C-12 CHIMPS2 data, we estimate a median optical depth of tau(13 )= 0.087. The preliminary analysis yields a median (CO)-C-13 column-density range equal to N((CO)-C-13) = 2-5 x 10(18)cm(-2), median H-2 column density equal to N(H-2) = 4x10(22)cm(-2) to 1x10(23)cm(-2). We derive N(H-2)-based total mass estimates of M(H-2) = 2-6x10(7)M(circle dot), in agreement with previous studies. We analyse the relationship between the integrated intensity of (CO)-C-13 and the surface density of compact sources identified by Herschel Hi-GAL, and find that younger Hi-GAL sources detected at 500 mu m but not at 70 mu m follow the dense gas of the CMZ more closely than those that are bright at 70 mu m. The latter, actively star-forming sources appear to be more associated with material in the foreground spiral arms
WOS关键词C-12/C-13 ISOTOPE RATIO ; GALACTIC STAR-FORMATION ; 1ST DATA RELEASE ; INTERSTELLAR-MEDIUM ; LINE SURVEY ; MILKY-WAY ; GAS ; CLOUDS ; ABUNDANCES ; MASS
资助项目Science and Technology Facilities Council of the United Kingdom
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001285375900004
出版者OXFORD UNIV PRESS
资助机构Science and Technology Facilities Council of the United Kingdom
源URL[http://ir.xao.ac.cn/handle/45760611-7/6904]  
专题恒星形成与演化研究团组
通讯作者King, S. M.; Moore, T. J. T.; Eden, D. J.
作者单位1.Chinese Acad Sci, Purple Mt Observ, Nanjing 210034, Peoples R China
2.Univ Alberta, Dept Phys, Edmonton, AB T6G 2E1, Canada
3.Univ Leeds, Sch Phys & Astron, Leeds LS2 9JT, England
4.Armagh Observ & Planetarium, Coll Hill, Armagh BT61 9DB, North Ireland
5.Liverpool John Moores Univ, Astrophys Res Inst, IC2,Liverpool Sci Pk,146 Brownlow Hill, Liverpool L3 5RF, England
6.Natl Taiwan Normal Univ, Ctr Astron & Gravitat, Dept Earth Sci, 88,Sec 4,Ting Chou Rd, Taipei 116, Taiwan
7.Natl Taiwan Normal Univ, Dept Earth Sci, 88 Sect 4,Ting Chou Rd, Taipei 11677, Taiwan
8.Acad Sinica, Inst Astron & Astrophys, 11F Astron Math Bldg,AS NTU 1,Sect 4,Roosevelt Rd, Taipei 10617, Taiwan
9.Shanghai Astron Observ, 80 Nandan Rd, Shanghai 200030, Peoples R China
10.Cardiff Univ, Sch Phys & Astron, 5 Parade,Newport Rd, Cardiff CF24 3AA, Wales
推荐引用方式
GB/T 7714
King, S. M.,Moore, T. J. T.,Henshaw, J. D.,et al. CHIMPS2: 13CO J=3→2 emission in the central molecular zone[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2024,533(1):131-142.
APA King, S. M..,Moore, T. J. T..,Henshaw, J. D..,Longmore, S. N..,Eden, D. J..,...&Rani, R..(2024).CHIMPS2: 13CO J=3→2 emission in the central molecular zone.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,533(1),131-142.
MLA King, S. M.,et al."CHIMPS2: 13CO J=3→2 emission in the central molecular zone".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 533.1(2024):131-142.

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