Observing the Evolution of Disk Galaxies

Physics – Optics

Scientific paper

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Scientific paper

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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