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Studies of NGC 6720 with Calibrated HST/WFC3 Emission-line Filter Images. II. Physical Conditions

  • Authors: C. R. O'Dell, G. J. Ferland, W. J. Henney, and M. Peimbert

O'Dell et al. 2013 The Astronomical Journal 145 93.

  • Provider: AAS Journals

Caption: Figure 8.

This image of the derived equivalent width of the Hβ emission line is for the same FOV as Figure 3 of the preceding paper. The stitching caused by the dithering across the gap between the two CCDs is even more obvious, but does not affect the derived equivalent width. The positive Y-axis points toward P.A. = 335°. The variations in the equivalent width are discussed in the text.

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