to IAU
Symposium 241
Symposium 241
Abstract details
The Stellar Populations in the Outer Banks of Massive Disk Galaxies
Abstract
In recent years we have started to appreciate that the outer banks of
galaxies contain valuable information about the formation process of
galaxies. In hierarchical galaxy formation the stellar halos and thick
disks of galaxies are formed by accretion of minor satellites,
predominantly in the earlier assembly phases. The size, metallicity,
and amount of substructure in current day halos are therefore directly
related to issues like the small scale properties of the primordial
power spectrum of density fluctuations and the suppression of star
formation in small dark matter halos after reionization.
I will show initial results from our ongoing HST/ACS survey of the
resolved stellar populations of 14 nearby, massive disk galaxies. I
will show that the smaller galaxies have no significant halo. I will present
the stellar populations of a very low surface brightness stream around
M83, the first such a stream resolved into stars beyond those of the
Milky Way and M31. Finally, I will show that the old RGB stars of the
thick disk in an edge-on galaxy truncate at the same radius as the
young thin disk stars, providing insights into the formation of both
disk truncations and thick disks.