Baryons and dark matter halo distributions in ACDM cosmology

Susana Pedrosa, Patricia Tissera, Cecilia Scannapieco

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

Resumen

We analyse the dark matter (DM) distribution in a ≈ 10 M alo extracted from a simulation consistent with the concordance cosmology, where the physics regulating the transformation of gas into stars was allowed to change producing galaxies with different morphologies. Although the DM profiles get more concentrated as baryons are collected at the centre of the haloes compared to a pure dynamical run, the total baryonic mass alone is not enough to fully predict the reaction of the DM profile. Our findings suggest that the response of the DM halo is driven by the history of assembly of baryons into a galaxy. The accretion of satellites could be associated with an expansion of the dark matter profiles, triggered by angular momentum transfer from the incoming satellites. However, we also found that these mechanism have different efficiencies which are set by the history of formation of the structure.

Idioma originalInglés
Páginas (desde-hasta)404-405
Número de páginas2
PublicaciónProceedings of the International Astronomical Union
Volumen5
N.ºS262
DOI
EstadoPublicada - ago 2009

Áreas temáticas de ASJC Scopus

  • Medicina (miscelánea)
  • Astronomía y astrofísica
  • Nutrición y dietética
  • Salud pública, medioambiental y laboral
  • Ciencias planetarias y espacial

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