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Fig. 10.

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Median radial profiles of physical quantities of 30 random galaxies (10 random galaxies for each size class) that end up as centrals at different epochs: radial velocity of the gas (first row), gas specific angular momentum normalized by the radius (second row), gas density times r2 (third row), sSFR (fourth row), and stellar density times r2 (fifth row). The r values have been converted to physical kiloparsecs. The colors are the same as in Fig. 3. The pink shaded regions indicate the redshift-dependent, poorly resolved radii and the dashed vertical lines indicate the redshift-dependent stellar half-mass radius.

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