Galactic accretion and the outer structure of galaxies in the CDM model

We have combined the semi-analytic galaxy formation model of Guo et al. with the particle-tagging technique of Cooper et al. to predict galaxy surface brightness profiles in a representative sample of ∼1900 massive dark matter haloes (1012-1014M) from the Millennium II Λ cold dark matter N-body simu...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2013-10, Vol.434 (4), p.3348-3367
Hauptverfasser:	Cooper, Andrew P., D'Souza, Richard, Kauffmann, Guinevere, Wang, Jing, Boylan-Kolchin, Michael, Guo, Qi, Frenk, Carlos S., White, Simon D. M.
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Dark matter Simulation Stars & galaxies
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