MOND and the fundamental plane of elliptical galaxies

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dc.creatorScarpa, Riccardo
dc.date2003-02-21
dc.date.accessioned2026-07-07T02:07:41Z
dc.date.available2026-07-07T02:07:41Z
dc.descriptionIt 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.
dc.descriptionPresented at the "Structure Evolution and Cosmology" symposium, held on October 2002, at E.S.O., Santiago, Chile. Includes 16 pages + 8 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0302445
dc.identifierhttp://arxiv.org/abs/astro-ph/0302445
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5776
dc.subjectAstrophysics
dc.titleMOND and the fundamental plane of elliptical galaxies
dc.typetext

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