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Resolving the Stellar Populations in the Circumnuclear Ring of NGC 7469

  • Authors: T. Díaz-Santos, A. Alonso-Herrero, L. Colina, S. D. Ryder, and J. H. Knapen

Díaz‐Santos et al. 2007 The Astrophysical Journal 661 149.

  • Provider: AAS Journals

Caption: Fig. 2.

Contours, shown in a logarithmic scale, representing the HST NICMOS F110W emission. The 1.1 μm–selected star clusters are marked with small open circles with sizes equivalent to the FWHM of the F110W PSF (sime37 pc; see Table 1). The location and P.A. of the UKIRT CGS4 slits are also marked, with the ﹩0.6^{\prime \prime }﹩ slit width and extraction lengths (see Table 4) shown to scale. The ring area defined by G95 (enclosed by two open circles of radii ﹩0.7^{\prime \prime }﹩ and ﹩2.5^{\prime \prime }﹩; see text) is also shown. North is up, and east to the left.

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