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KMOS^3D: Dynamical constraints on the mass budget in early star-forming disks

, , , , , , , , , , , , , , , , , , , , , , , , , , , , and . (2016)cite arxiv:1603.03432Comment: Submitted to ApJ. Fig. 4 compares stellar and baryonic masses to dynamical masses. Fig. 6 and 7 show the dependence of stellar and baryonic mass fractions on redshift and surface density.

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