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Chinese Academy of Sciences Institutional Repositories Grid
Dense gas in the Galactic central molecular zone is warm and heated by turbulence

文献类型:期刊论文

作者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
刊名ASTRONOMY & ASTROPHYSICS
出版日期2016-02-01
卷号586
关键词Galaxy: center ISM: molecules ISM: structure Galaxy: nucleus cosmic rays ISM: clouds
英文摘要Context. The Galactic center is the closest region where we can study star formation under extreme physical conditions like those in high-redshift galaxies.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]STAR-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
收录类别SCI
语种英语
WOS记录号WOS:000369715900061
源URL[http://libir.pmo.ac.cn/handle/332002/16148]  
专题紫金山天文台_分子云与恒星形成研究团组
作者单位1.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
推荐引用方式
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).

入库方式: OAI收割

来源:紫金山天文台

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