The growth of galactic bulges through mergers in LCDM haloes revisited. I. Present-day properties

Jesus Zavala Franco, Vladimir Avila-Reese, Claudio Firmani, Michael Boylan-Kolchin

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Abstract

We use the Millennium I and II cosmological simulations to revisit the impact of mergers in the growth of bulges in central galaxies in the LCDM scenario. We seed galaxies within the growing CDM haloes using semi-empirical relations to assign stellar and gaseous masses, and an analytic treatment to estimate the transfer of stellar mass to the bulge of the remnant after a galaxy merger. We find that this model roughly reproduces the observed correlation between the bulge-to-total (B/T) mass ratio and stellar mass in present-day central galaxies as well as their observed demographics, although low-mass B/T
OriginalsprogEngelsk
TidsskriftMonthly Notices of the Royal Astronomical Society
Vol/bind427
Udgave nummer2
Sider (fra-til)1503-1516
ISSN0035-8711
DOI
StatusUdgivet - 2012
Udgivet eksterntJa

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