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The equilibrium structure of cosmological halos: from dwarf galaxies to x-ray clusters
A new model for the postcollapse equilibrium structure of virialized objectswhich condense out of the cosmological background universe is described and com-pared with observations and simulations of cosmological halos. The model is basedupon the assumption that virialized halos are isothermal, which...
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| Publicado no: | Revista Mexicana de Astronomía y Astrofísica |
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| Main Authors: | , |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Universidad Nacional Autónoma de México
2001
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| Assuntos: | |
| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57101032 |
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