Mergers between elliptical galaxies and the thickening of the Fundamental Plane
[EN]We have carried out computer simulations to study the effect of merging on the Fundamental Plane (FP) relation. Initially, systems are spherical Jaffe models following a simple scaling relation (M/R2e= constant). They have been put on the FP by imposing different M/L values. Various orbital char...
| Autores: | , |
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| Tipo de recurso: | artículo |
| Fecha de publicación: | 2003 |
| País: | España |
| Institución: | Consejo Superior de Investigaciones Científicas (CSIC) |
| Repositorio: | DIGITAL.CSIC. Repositorio Institucional del CSIC |
| OAI Identifier: | oai:digital.csic.es:10261/75013 |
| Acceso en línea: | http://hdl.handle.net/10261/75013 |
| Access Level: | acceso abierto |
| Palabra clave: | Methods: N-body simulations Galaxies: elliptical and lenticular, cD Galaxies: fundamental parameters Galaxies: interactions Incipit Institute of Heritage Sciences Instituto de Ciencias del Patrimonio |
| Sumario: | [EN]We have carried out computer simulations to study the effect of merging on the Fundamental Plane (FP) relation. Initially, systems are spherical Jaffe models following a simple scaling relation (M/R2e= constant). They have been put on the FP by imposing different M/L values. Various orbital characteristics have been considered. Our results show that the merger remnants lie very close to the FP of the progenitors. Although non-homology is introduced by the merging process, mergers among homologous galaxies leave a pre-existing FP-relation intact. As a side result we find that variations in the point of view lead to non-negligible scatter about the FP. |
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