Consequences of the external field effect for MOND disc galaxies in galaxy clusters-Reference-Cited by-同舟云学术

Consequences of the external field effect for MOND disc galaxies in galaxy clusters

Published:2018-08-16 Issue:4 Volume:480 Page:5362-5379
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Candlish G N¹,Smith R²,Jaffé Y¹,Cortesi A³

Affiliation:

1. Instituto de Física y Astronomía, Universidad de Valparaíso, Gran Bretaña 1111, Valparaíso, Chile

2. Korea Astronomy and Space Science Institute, 766, Daedeokdae-ro, Yuseon-gu, Daejon 34055, Korea

3. Departamento de Astronomia, Instituto de Astronomia, Geofisica e Ciencias Atmosfericas da USP, Cidade Universitaria, CEP:05508900, Sao Paulo, SP, Brazil

Funder

Consejo Nacional de Innovación, Ciencia y Tecnología

Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica

Conselho Nacional de Desenvolvimento Científico e Tecnológico

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/480/4/5362/25636735/sty2228.pdf

Reference62 articles.

1. Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A

2. Modified Newtonian Dynamics (MOND) as a Modification of Newtonian Inertia

3. The abundance of galaxy clusters in modified Newtonian dynamics: cosmological simulations with massive neutrinos

4. Relativistic gravitation theory for the modified Newtonian dynamics paradigm

5. Does the missing mass problem signal the breakdown of Newtonian gravity?

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