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On the Evolution of the Central Density of Quiescent Galaxies

  • Authors: Sandro Tacchella, C. Marcella Carollo, S. M. Faber, Anna Cibinel, Avishai Dekel, David C. Koo, Alvio Renzini, and Joanna Woo

2017 The Astrophysical Journal Letters 844 L1.

  • Provider: AAS Journals

Caption: Figure 4.

At a given M, QGs with a higher Σ1 are older. We plot Σ1 vs. M for QGs, color coded by the three mass-weighted age bins of Figure 3. Galaxies above the Σ1 ridgeline, indicated with the black line, are older than similar-mass galaxies below this line. The inset shows the distribution of distances from the Σ1 ridgeline for the three age categories.

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