Schedule Sep 29, 2008
Bulgeless Disks in Hydrodynamic Cosmological Simulations
Chris Brook (Univ. Washington)

We form a bulgeless dwarf disk galaxy with linearly rising rotation curve in a full hydrodynamic cosmological galaxy formation simulation. The importance of feedback and the ability to better resolve star forming regions are highlighted. Implications for the next generation of Milky Way simulations are then discussed, and results from the latest, highest resolution simulated Milky Way galaxy are presented. A theme will be the relative importance of accreted versus in situ populations for each of the main components of the Milky Way.

Begin streaming QuickTime of the whole talk (high bandwidth).
(Or, right-click to download the movie.) (Or, right-click to download the podcast.)

Begin streaming RealMedia for the whole talk: high bandwidth or medium bandwidth.
Or, stream audio only for the whole talk: high bandwidth or low bandwidth. (Or, right-click to download the whole audio file.)

To begin viewing slides, click on the first slide below. (Or, view as pdf.)


[01] [02] [03] [04] [05] [06] [07] [08] [09] [10] [11] [12] [13] [14] [15] [16] [17] [18] [19] [20] [21] [22] [23] [24] [25] [26] [27] [28] [29] [30] [31]

Author entry (protected)