Analysis of galaxy formation with hydrodynamics

Patricia B. Tissera, Diego G. Lambas, Mario G. Abadi

Resultado de la investigación: Contribución a una revistaArtículorevisión exhaustiva

46 Citas (Scopus)

Resumen

We present a hydrodynamical code based on the smoothed particle hydrodynamics (SPH) technique implemented in an APSM code that is aimed at solving the hydrodynamical and gravitational equations in a cosmological frame. We analyse the ability of the code to reproduce standard tests and perform numerical simulations to study the formation of galaxies in a typical region of a cold dark matter (CDM) model. These numerical simulations include gas and dark matter particles and take into account physical processes such as shock waves, radiative cooling and a simplified model of star formation. We analyse the astrophysical properties of the galactic objects in different models.

Idioma originalInglés
Páginas (desde-hasta)384-392
Número de páginas9
PublicaciónMonthly Notices of the Royal Astronomical Society
Volumen286
N.º2
DOI
EstadoPublicada - 1997

Áreas temáticas de ASJC Scopus

  • Astronomía y astrofísica
  • Ciencias planetarias y espacial

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