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Fig. 12

image

Specific angular momentum of disks jd as a function of galaxy stellar mass for the MUSE-HDFS sample of spatially resolved galaxies. Data points are color-coded according to the V/σ ratio. Diamond outlines indicate dispersion-dominated galaxies with V/σ< 1. The dashed lines show the relations defined for massive galaxies at z = 0 (Fall & Romanowsky 2013), distinguishing between spheroids (red line, M> 1010M) and disks (blue line, M> 109M).

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