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The Structure and Metallicity Gradient in the Extreme Outer Disk of NGC 7793

  • Authors: M. Vlajić, J. Bland-Hawthorn, and K. C. Freeman

Vlajić, Bland-Hawthorn, & Freeman 2011 The Astrophysical Journal 732 7.

  • Provider: AAS Journals

Caption: Figure 3.

CMD of two NGC 7793 fields. Dashed lines represent the 50% completeness limit. Photometric uncertainties at a given magnitude and color of g′ − i′ = 1 are shown on the left of the panels.

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