| Revista: | Brazilian journal of physics |
| Base de datos: | PERIÓDICA |
| Número de sistema: | 000335827 |
| ISSN: | 0103-9733 |
| Autors: | Fabris, J.C1 Velten, H.E.S1 |
| Institucions: | 1Universidade Federal do Espirito Santo, Departamento de Fisica, Vitoria, Espirito Santo. Brasil |
| Any: | 2009 |
| Període: | Sep |
| Volum: | 39 |
| Número: | 3 |
| Paginació: | 592-595 |
| País: | Brasil |
| Idioma: | Inglés |
| Tipo de documento: | Artículo |
| Enfoque: | Experimental, analítico |
| Resumen en inglés | Large values for the mass-to-light ratio (ϒ) in self-gravitating systems is one of the most important evidences of dark matter. We propose a expression for the mass-to-light ratio in spherical systems using MOND. Results for the COMA cluster reveal that a modification of the gravity, as proposed by MOND, can reduce significantly this value |
| Disciplines | Física y astronomía |
| Paraules clau: | Astronomía, Sistemas autogravitacionales, Materia oscura, Proporción masa-luz |
| Keyword: | Physics and astronomy, Astronomy, Self-gravitating systems, Dark matter, Mass-light ratio |
| Text complet: | Texto completo (Ver HTML) |
