PMO OpenIR  > 分子云与恒星形成研究团组
Dense gas in the Galactic central molecular zone is warm and heated by turbulence
Ginsburg, Adam1; Henkel, Christian2,3; Ao, Yiping4,5; Riquelme, Denise2; Mann, Jens Kau Ff2; Pillai, Thushara2; Mills, Elisabeth A. C.6; Requena-Torres, Miguel A.2; Immer, Katharina1; Testi, Leonardo1; Ott, Juergen6; Bally, John7; Battersby, Cara8; Darling, Jeremy7; Aalto, Susanne9; Stanke, Thomas1; Kendrew, Sarah10; Kruijssen, J. M. Diederik11; Longmore, Steven12; Dale, James13; Guesten, Rolf2; Menten, Karl M.2
2016-02-01
Source PublicationASTRONOMY & ASTROPHYSICS
Volume586
AbstractContext. The Galactic center is the closest region where we can study star formation under extreme physical conditions like those in high-redshift galaxies.
KeywordGalaxy: Center Ism: Molecules Ism: Structure Galaxy: Nucleus Cosmic Rays Ism: Clouds
WOS HeadingsScience & Technology ; Physical Sciences
DOI10.1051/0004-6361/201526100
WOS KeywordSTAR-FORMATION RATE ; CENTER CLOUD G0.253+0.016 ; SGR A-ASTERISK ; INFRARED-DARK CLOUDS ; MILKY-WAY ; INTERSTELLAR-MEDIUM ; ASTROPHYSICAL MEDIA ; PHYSICAL-PROPERTIES ; SAGITTARIUS B2 ; CENTER REGION
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000369715900061
Citation statistics
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/16148
Collection分子云与恒星形成研究团组
Affiliation1.European So Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany
2.Max Planck Inst Radio Astron, D-53121 Bonn, Germany
3.King Abdulaziz Univ, Dept Astron, POB 80203, Jeddah 21589, Saudi Arabia
4.Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan
5.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
6.Natl Radio Astron Observ, Socorro, NM 87801 USA
7.Univ Colorado, CASA, 389 UCB, Boulder, CO 80309 USA
8.Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
9.Chalmers, Dept Earth & Space Sci, S-41258 Gothenburg, Sweden
10.Univ Oxford, Dept Astrophys, Denys Wilkinson Bldg,Keble Rd, Oxford OX1 3RH, England
11.Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85748 Garching, Germany
12.Liverpool John Moores Univ, Astrophys Res Inst, IC2,Liverpool Sci Pk,146 Brownlow Hill, Liverpool L3 5RF, Merseyside, England
13.Univ Observ Munich, Scheinerstr 1, D-81679 Munich, Germany
Recommended Citation
GB/T 7714
Ginsburg, Adam,Henkel, Christian,Ao, Yiping,et al. Dense gas in the Galactic central molecular zone is warm and heated by turbulence[J]. ASTRONOMY & ASTROPHYSICS,2016,586.
APA Ginsburg, Adam.,Henkel, Christian.,Ao, Yiping.,Riquelme, Denise.,Mann, Jens Kau Ff.,...&Menten, Karl M..(2016).Dense gas in the Galactic central molecular zone is warm and heated by turbulence.ASTRONOMY & ASTROPHYSICS,586.
MLA Ginsburg, Adam,et al."Dense gas in the Galactic central molecular zone is warm and heated by turbulence".ASTRONOMY & ASTROPHYSICS 586(2016).
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