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Stéphane Courteau

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Ascona/Terschelling Highlights<br />

What is the origin of this disk truncation - common and seen<br />

more easily in edge-on galaxies than in face-on galaxies<br />

Kregel etal (2002):<br />

R max/h R = 3.6 ± 0.6<br />

for 34 edge-on disk<br />

galaxies<br />

Perez (2004) finds<br />

similar results at<br />

0.6

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