| |
 |
| Paper: |
The Elaboration of Spiral Galaxies: Morpho-Kinematics Analyses of their Progenitors with IMAGES |
| Volume: |
419, Galaxy Evolution: Emerging Insights and Future Challenges |
| Page: |
66 |
| Authors: |
Hammer, F.; IMAGES Collaboration |
| Abstract: |
The IMAGES (Intermediate MAss Galaxy Evolution Sequence) project aims at measuring the velocity fields of a representative sample of 100 massive galaxies at z=0.4–0.75, selected in the CDFS, the CFRS and the HDFS fields. It uses the world-unique mode of multiple integral field units of FLAMES/ GIRAFFE at VLT. The resolved-kinematics data allow us to sample the large scale motions at ∼ few kpc scale for each galaxy. They have been combined with the deepest HST/ACS, Spitzer (MIPS and IRAC) and VLT/FORS2 ever achieved observations. Most intermediate redshift galaxies show anomalous velocity fields: 6 Gyrs ago, half of the present day spirals were out of equilibrium and had peculiar morphologies.
The wealth of the data in these fields allow us to modelize the physical processes
in each galaxy with an accuracy almost similar to what is done in the local
Universe. These detailed analyses reveal the importance of merger processes,
including their remnant phases. Together with the large evolution of spiral
properties, this points out the importance of disk survival and strengthens the
disk rebuilding scenario. This suggests that the hierarchical scenario may apply
to the elaboration of disk galaxies as it does for ellipticals. |
|
|
|
|
|
