Fig. 17
Radial distribution of specific angular momentum. Panel a: adapted from Fig. 8 of Belloche (2013) and from Ohashi et al. (1997a). Panel b: zoom on the region where the angular momentum profiles due to rotation of the CALYPSO sources lie. The gray curve shows the median profile j(r). In the two panels, the solid black line shows the best fit with a broken power-law model.
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