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SEEDING THE LOCAL DISK GALAXY POPULATION

By means of the abundance matching technique we have inferred the local stellar & baryonic-halo mass (Ms & Mb - Mh) relations for central blue and red galaxies. Models of disk galaxies loaded inside A Cold Dark Matter (ACDM) halos are used to probe the obtained blue Mb -Mh relation in the light of o...

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Bibliográfalaš dieđut
Publikašuvnnas:Revista Mexicana de Astronomía y Astrofísica
Váldodahkkit: A. Rodríguez-Puebla, V. Avila-Reese, C. Firmani, P. Colín
Materiálatiipa: Artigo
Giella:Inglês
Almmustuhtton: Universidad Nacional Autónoma de México 2011
Fáttát:
Liŋkkat:https://www.redalyc.org/articulo.oa?id=57121297035
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