Stéphane Courteau
Stéphane Courteau
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