Astronomy and Astrophysics – Astrophysics
Scientific paper
1998-12-10
Astronomy and Astrophysics
Astrophysics
19 pages, 6 figures, accepted for publication in the Astrophysical Journal
Scientific paper
10.1086/307096
In this paper, we present three qualitatively different scenarios for bulge formation: a secular evolution model in which bulges form after disks and undergo several central starbursts, a primordial collapse model in which bulges and disks form simultaneously, and an early bulge formation model in which bulges form prior to disks. We normalize our models to the local z=0 observations of de Jong & van der Kruit (1994) and Peletier & Balcells (1996) and make comparisons with high redshift observations. We consider model predictions relating directly to bulge-to-disk properties. As expected, smaller bulge-to-disk ratios and bluer bulge colors are predicted by the secular evolution model at all redshifts, although uncertainties in the data are currently too large to differentiate strongly between the models.
Bouwens Rychard J.
Cayón Laura
Silk Joseph
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