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Bodo Ziegler

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<strong>Bodo</strong> <strong>Ziegler</strong>: Kinematic & Structural Evolution of Field & Cluster Spirals - Potsdam 21.9.10<br />

Morphologies of distant galaxies<br />

Fit 2dim surface brightness with your favorite<br />

➔ law (exponential, Sersic etc) for disk & bulge<br />

➔ model package (GALFIT, GIM2D, BUDDA)<br />

or use your favorite non-parametric approach<br />

➔ CAS: concentration, asymmetry, clumpiness<br />

➔ Gini & M 20<br />

⇒ structure evolution<br />

z=0.5 spiral<br />

GALFIT<br />

disk+bulge<br />

● What defines the morphology of a galaxy?

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