MOND virial theorem applied to a galaxy cluster
dc.date.accessioned | 2011-04-04T20:08:19Z | |
dc.date.available | 2011-04-04T20:08:19Z | |
dc.identifier.citation | FABRIS, J. C.; VELTEN, H. E. S. MOND virial theorem applied to a galaxy cluster. Braz. J. Phys., São Paulo, v. 39, n. 3, p. 592-595, set. 2009. Disponível em: <http://www.scielo.br/pdf/bjp/v39n3/15.pdf>. Acesso em: 31 mar. 2011. | por |
dc.identifier.doi | 10.1590/S0103-97332009000500015 | |
dc.identifier.issn | 0103-9733 | |
dc.identifier.uri | http://repositorio.ufes.br/handle/10/660 | |
dc.rights | open access | en |
dc.title | MOND virial theorem applied to a galaxy cluster | por |
dc.type | article | en |
dcterms.abstract | 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. | eng |
dcterms.creator | Fabris, Júlio César | |
dcterms.creator | Velten, Hermano Endlich Schneider | |
dcterms.issued | 2009-09 | |
dcterms.language | eng | en |
dcterms.subject | Galáxias - Aglomerados | por |
dcterms.subject | Matéria escura (Astronomia) | por |
dcterms.subject | MOND | eng |
dcterms.subject | COMA cluster | eng |
dcterms.subject | Dark Matter | eng |
dcterms.subject | Galaxies - Clusters | eng |