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Rapid Bulge Assembly in Young Galaxy Disks at Cosmic Dawn

  • Authors: Anshuman Borgohain, Kanak Saha

Anshuman Borgohain and Kanak Saha 2026 The Astrophysical Journal Supplement Series 287 .

  • Provider: AAS Journals

Caption: Figure 5.

A comparison of global galaxy properties z ≥ 6 galaxy sample with lower-redshift CANDELS galaxies from P. Dimauro et al. (2018). The gray-shaded histograms show the distributions for all galaxies in our sample, while the solid black histograms represent the subset of galaxies identified with two components. The blue-dashed and red-dotted histograms show the distributions for CANDELS SF and quiescent (Q) galaxies at 0 < z < 3, respectively. (a) A distribution of stellar-mass surface density, ﹩{{\rm{\Sigma }}}_{\mathrm{Re}}﹩ calculated within circularized Re. (b) A distribution of star formation timescales, τSF. (c) A distribution of star formation rate surface density, ΣSFR.

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