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2010MNRAS.403..768H - Mon. Not. R. Astron. Soc., 403, 768-779 (2010/April-1)
Tidal disruption of satellite galaxies in a semi-analytic model of galaxy formation.
HENRIQUES B.M.B. and THOMAS P.A.
Abstract (from CDS):
To test the significance of the new physical process, we apply a Monte Carlo Markov Chain parameter estimation technique constraining the model with the K-band luminosity function, B - V colours and the black hole-bulge mass relation. The differences in parameter correlations, and in the allowed regions in likelihood space, reveal the impact of the new physics on the basic ingredients of the model, such as the star formation laws, feedback recipes and the black hole growth model.
With satellite disruption in place, we get a model likelihood four times higher than in the original model, indicating that the new process seems to be favoured by observations. This is achieved mainly due to a reduction in black hole growth that produces a better agreement between the properties of central black holes and host galaxies. Compared to the best-fitting model without disruption, the new model removes the excess of dwarf galaxies in the original recipe with a more modest supernova heating.
The new model is now consistent with the three observational data sets used to constrain it, while significantly improving the agreement with observations for the distribution of metals in stars. Moreover, the model now has predictions for the intra-cluster light, a very significant component of large groups and clusters, that agree with observational estimates.
Abstract Copyright: © 2010 The Authors. Journal compilation © 2010 RAS
Journal keyword(s): methods: numerical - methods: statistical - galaxies: evolution - galaxies: formation
Simbad objects: 3
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