A modification of the Newtonian dynamics - Implications for galaxies
about
Balance of Dark and Luminous Mass in Rotating GalaxiesRelativistic gravitation theory for the modified Newtonian dynamics paradigmPhoton and graviton mass limitsRunning Newton constant, improved gravitational actions, and galaxy rotation curvesProbing Gravity at Cosmological Scales by Measurements which Test the Relationship between Gravitational Lensing and Matter OverdensityReduced time delay for gravitational waves with dark matter emulatorsModel of dark matter and dark energy based on gravitational polarizationIs Violation of Newton’s Second Law Possible?A dynamical model of the local cosmic expansionModified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic ExtensionsExperimental Searches for Dark MatterDark matter universe.Dark matter.A gravitational diffusion model without dark matter.The Pioneer AnomalyTensor-vector-scalar-modified gravity: from small scale to cosmology.Quantum-Spacetime PhenomenologyDynamical boson stars.Radial Acceleration Relation in Rotationally Supported Galaxies.Large Scale Structure in Bekenstein’s Theory of Relativistic Modified Newtonian DynamicsThe modified Newtonian dynamics—MOND and its implications for new physicsPhenomenological covariant approach to gravityGravitational analysis of V541 Cygni, DI Herculis, and the Pioneer anomalyFirst test of Verlinde's theory of emergent gravity using weak gravitational lensing measurementsCan Cosmic Structure Form without Dark Matter?A historical perspective on modified Newtonian dynamicsThe origin of the mass discrepancy–acceleration relation in ΛCDMThe Anatomy of GalaxiesEstimating non-circular motions in barred galaxies using numericalN-body simulationsEvolution of spiral galaxies in modified gravityLaboratory Test of Newton’s Second Law for Small AccelerationsA tale of two paradigms: the mutual incommensurability of ΛCDM and MONDDetecting a Lorentz-violating field in cosmologyTesting alternative theories of dark matter with the CMBCosmological behavior of Bekenstein’s modified theory of gravityGalaxy clusters in the context of superfluid dark matterEmergent gravity in galaxies and in the Solar SystemUnderstanding the internal dynamics of elliptical galaxies without non-baryonic dark matterCombined Solar system and rotation curve constraints on MONDRemarks on the properties of elliptical galaxies in modified Newtonian dynamics
P2860
Q21563691-B3D4751E-423D-4FC2-9DF0-5BF7ADA9B2A4Q21707318-EE4B07D2-C7D1-4256-B5FC-EFDDE0522A97Q22065728-F25F1BAE-D15E-400F-962C-FA0264156A93Q27349461-460A27C5-B033-491A-850A-2876D608408DQ27349798-BEDEC143-8040-4043-8E78-F33C3F9CD98BQ27442322-5D9BE46E-B7AA-4C94-9038-A31632A3FC90Q27442398-4F568F80-17E5-464E-8DB9-C711C7465B62Q27454493-CFBAB505-DBA1-4BBE-9CF0-020370061A08Q28315170-4F5BEFC5-4EFF-494E-BE4C-9FAADECFB4B6Q30364179-390E2E62-87B6-496E-A47B-ED890D685688Q30364208-32709A14-3115-4FD8-8197-2D0BC2805FD6Q30401057-CA1E3BFE-E8A0-453E-96BC-C8702CA49407Q30401060-C5B65012-3DB2-4804-8E72-3B6B78998F09Q35999819-230AB014-4A49-4322-9E47-1B6F0660935BQ36271070-93C8E793-046D-48A8-A68C-4049AFE9D6E5Q37956263-87F4E968-4D84-437C-9AF4-699AA18BB181Q38970932-FBE9690F-1F32-4581-91B4-8AE7A1B53445Q46772008-CEF1E1DB-4448-45D5-8BED-B8B830B472B5Q55059940-0DA812BC-A608-4353-A0E8-9E06DC125C6DQ55896440-8BF80A79-FEE6-4E54-9B30-39633DF04DC6Q55954092-12B8219B-8A9F-47D3-8A53-7A35B4C502C2Q56004026-28651A36-1C08-4415-AD91-B8CF931FDD18Q56032501-F9E07E81-FF52-4362-A243-2BEC4BB78BDBQ56041978-BAE4E656-36A1-4DAB-9919-F5A0E689AF5EQ56168592-B707B5B0-BD48-4872-9195-0BA65D79D41CQ56387634-503C43E3-3C76-4D44-94DC-AF2F1131E666Q56907258-BF624451-C2D4-4B8F-A834-1872E2D32AF5Q56914181-5C5474C8-C97E-448C-9846-9C2B2B15E04EQ56914207-8A88F434-5805-4FE3-90B5-4CCC943DDAA0Q56915631-DA1DFE09-C908-429B-AC5C-FA385FE22FA3Q57311817-70BDC454-4C3D-4A40-8D16-42B5881BE3AEQ57486364-B5FB796E-6B03-4723-BACF-F04A81A8764EQ58200815-561DA120-6B01-4EB5-83E0-0C1CA1EA0FC2Q58200845-F004459F-1BE5-404E-8E48-C26D4BF5101EQ58200859-38FFEB4A-354C-4156-94FB-A3E08C5B6AC6Q58328487-09303DAE-5ADB-423A-91F5-0BF3731FDFEDQ58328499-3F6835D0-F0D5-472F-ABFD-E30668339E68Q58328506-60855B0F-4595-45D8-B43F-5981A3388AE7Q58328519-A27B4837-3235-40C6-B5FD-732872D00ECEQ58328590-84C97AFB-12BA-4A54-9F83-EF5E8AB1C1AD
P2860
A modification of the Newtonian dynamics - Implications for galaxies
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Juli 1983 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в липні 1983
@uk
name
A modification of the Newtonian dynamics - Implications for galaxies
@en
A modification of the Newtonian dynamics - Implications for galaxies
@nl
type
label
A modification of the Newtonian dynamics - Implications for galaxies
@en
A modification of the Newtonian dynamics - Implications for galaxies
@nl
prefLabel
A modification of the Newtonian dynamics - Implications for galaxies
@en
A modification of the Newtonian dynamics - Implications for galaxies
@nl
P356
P1476
A modification of the Newtonian dynamics - Implications for galaxies
@en
P2093
M. Milgrom
P304
P356
10.1086/161131
P407
P577
1983-07-01T00:00:00Z
P819
1983ApJ...270..371M