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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 2.

Extinction factor c is shown as derived from the observed Hα/Hβ ratio and assuming an intrinsic ratio of 2.87, which applies to a low density gas at T e = 10,000 K. The X-axis lies along P.A. = 240° and the Y-axis along P.A. = 330°. The sample was 4'' wide and the data have been averaged along bins of 10 pixels, corresponding to 0 farcs4. The distance shown is from the position of the central star. The data closest to that star have been edited out because of contamination, thus causing a central gap or in later similar images, artificial values near the central star.

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