MOND and the fundamental plane of elliptical galaxies

Details MOND and the fundamental plane of elliptical galaxies MOND and the fundamental plane of elliptical galaxies

2003-02-21

arxiv.org/abs/astro-ph/0302445v1

Astronomy and Astrophysics

Astrophysics

Presented at the "Structure Evolution and Cosmology" symposium, held on October 2002, at E.S.O., Santiago, Chile. Includes 16

Scientific paper

It is shown that the MOdified Newtonian Dynamics (MOND) explains the tilt of
the fundamental plane of elliptical galaxies without the need of non-baryonic
dark matter. Results found for elliptical galaxies extends to globular clusters
and galaxy clusters, showing that MOND agrees with observations over 7 order of
magnitude in acceleration.

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