Does the galaxy NGC1052-DF2 falsify Milgromian dynamics?

被引：46

作者：

Kroupa, Pavel ^{[1
,2
]}

Haghi, Hosein ^{[1
,3
]}

Javanmardi, Behnam ^{[4
]}

Zonoozi, Akram Hasani ^{[1
,3
]}

Mueller, Oliver ^{[5
]}

Banik, Indranil ^{[6
]}

Wu, Xufen ^{[7
,8
]}

Zhao, Hongsheng ^{[6
,9
]}

Dabringhausen, Jorg ^{[2
]}

机构：

[1] Univ Bonn, Helmholtz Inst Strahlen & Kernphys, Bonn, Germany

[2] Charles Univ Prague, Fac Math & Phys, Astron Inst, Prague, Czech Republic

[3] Inst Adv Studies Basic Sci, Dept Phys, Zanjan, Iran

[4] Inst Res Fundamental Sci IPM, Sch Astron, Tehran, Iran

[5] Univ Basel, Dept Phys, Basel, Switzerland

[6] Univ St Andrews, Scottish Univ Phys Alliance, St Andrews, Fife, Scotland

[7] Univ Sci & Technol China, Dept Astron, CAS Key Lab Res Galaxies & Cosmol, Hefei, Anhui, Peoples R China

[8] Univ Sci & Technol China, Sch Astron & Space Sci, Hefei, Anhui, Peoples R China

[9] Vrije Univ, Dept Phys & Astron, LaserLaB, Amsterdam, Netherlands

来源：

NATURE | 2018年 / 561卷 / 7722期

基金：

瑞士国家科学基金会; 安徽省自然科学基金;

关键词：

NEWTONIAN DYNAMICS; CLUSTERS;

D O I：

10.1038/s41586-018-0429-z

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

[No abstract available]

引用

页码：E4 / E5

页数：2

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