ANSWER TO MILGROM CRITICISMS

被引：0
|
作者：
GERBAL, D
DURRET, F
LACHIEZEREY, M
LIMANETO, G
机构：
[1] CE SACLAY, SERV ASTROPHYS, DAPNIA, F-91191 GIF SUR YVETTE, FRANCE
[2] CNRS, INST ASTROPHYS PARIS, F-75014 PARIS, FRANCE
[3] OBSERV PARIS, DEMIRM, URA 336, F-92195 MEUDON, FRANCE
来源：
ASTRONOMY & ASTROPHYSICS | 1993年 / 273卷 / 01期
关键词：
GALAXIES; CLUSTERING; (COSMOLOGY); DARK MATTER; LARGE-SCALE STRUCTURE OF UNIVERSE;
D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In a recent paper, we (Gerbal et al. 1992b) have applied MOdified Newtonian Dynamics to clusters of galaxies and have shown that in most cases the application of this theory is not sufficient to account for the dynamical properties of clusters, and that the presence of dark matter is still necessary. As a reply to the criticisms presented by Milgrom in a letter to A&A, we present here our answer to his letter.
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页码：L9 / L10
页数：2
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