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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 5.

Star counts profiles of the SE field (left panels) and NW field (right panels). From top to bottom, the profiles shown are of all stars (a and e), RGB (b and f), AGB (c and g), and MS stars (d and h). In each panel, the dashed line displays the estimated galaxy counts level, determined using methods described in the text. Open and full symbols show the star counts before and after the background galaxy contribution has been subtracted.

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