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Tidal dwarf galaxies as a test of fundamental physics

Tidal dwarf galaxies as a test of fundamental physics

http://www.wikidata.org/entity/Q56915867

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Modified Newtonian Dynamics (MOND): Observational Phenomenology and Relativistic Extensions Discrete clouds of neutral gas between the galaxies M31 and M33.Testing the MOND paradigm of modified dynamics with galaxy-galaxy gravitational lensing.THE FAILURES OF THE STANDARD MODEL OF COSMOLOGY REQUIRE A NEW PARADIGM Tidal dwarf galaxies in the nearby Universe A tale of two paradigms: the mutual incommensurability of ΛCDM and MOND Star formation triggered by galaxy interactions in modified gravity Phantom of RAMSES (POR): A new Milgromian dynamics N-body code A census of the expected properties of classical Milky Way dwarfs in Milgromian dynamics N-body simulations of the Carina dSph in MOND Local Group timing in Milgromian dynamics THINGS about MOND Galactic kinematics with modified Newtonian dynamics Milky Way potentials in cold dark matter and MOdified Newtonian Dynamics. Is the Large Magellanic Cloud on a bound orbit?Dwarf Galaxies, MOND, and Relativistic Gravitation Tidal Dwarf Galaxies and Missing Baryons

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Tidal dwarf galaxies as a test of fundamental physics

http://www.wikidata.org/entity/Q56915867

description

article publié dans la revue scientifique Astronomy and Astrophysics

@fr

im Juli 2007 veröffentlichter wissenschaftlicher Artikel

@de

scientific article published in Astronomy and Astrophysics

@en

wetenschappelijk artikel

@nl

наукова стаття, опублікована в липні 2007

@uk

name

Tidal dwarf galaxies as a test of fundamental physics

@en

Tidal dwarf galaxies as a test of fundamental physics

@nl

type

label

Tidal dwarf galaxies as a test of fundamental physics

@en

Tidal dwarf galaxies as a test of fundamental physics

@nl

prefLabel

Tidal dwarf galaxies as a test of fundamental physics

@en

Tidal dwarf galaxies as a test of fundamental physics

@nl

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0004-6361:20078081

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Astronomy and Astrophysics

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Tidal dwarf galaxies as a test of fundamental physics

@en

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G. Gentile

http://www.w3.org/2001/XMLSchema#string

H. S. Zhao

http://www.w3.org/2001/XMLSchema#string

O. Tiret

http://www.w3.org/2001/XMLSchema#string

P. Kroupa

http://www.w3.org/2001/XMLSchema#string

P2860

Missing mass in collisional debris from galaxies

Refining the MOND Interpolating Function and TeVeS Lagrangian

Formation of molecular gas in the tidal debris of violent galaxy-galaxy interactions.

Dwarf spheroidal satellites: are they of tidal origin?

The cored distribution of dark matter in spiral galaxies

Extended rotation curves of spiral galaxies: dark haloes and modified dynamics

A modification of the Newtonian dynamics as a possible alternative to the hidden mass hypothesis

Solutions for the modified Newtonian dynamics field equation

Modified Newtonian Dynamics and the "Dearth of Dark Matter in Ordinary Elliptical Galaxies"

Escaping from modified Newtonian dynamics

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25–28

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scholarly article

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10.1051/0004-6361:20078081

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2

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472

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Françoise Combes

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2007-07-23T00:00:00Z

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0706.1976

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2007A&A...472L..25G

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