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| Paper: |
Observing the Evolution of Disk Galaxies |
| Volume: |
379, Cosmic Frontiers |
| Page: |
344 |
| Authors: |
Tamm, A.; Tenjes, P. |
| Abstract: |
Imaging depth and resolution, made available by adaptive optics
and the HST, enable resolving galactic disks already at redshifts z ≈ 3. Rotation
curves can be obtained at up to z ≈ 1, allowing for the construction of self-consistent
mass distribution models. Examples of both cases are presented. |
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