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Extinction and Dust Geometry in M83 H II Regions: An Hubble Space Telescope/WFC3 Study

  • Authors: Guilin Liu, Daniela Calzetti, Sungryong Hong, Bradley Whitmore, Rupali Chandar, Robert W. O'Connell, William P. Blair, Seth H. Cohen, Jay A. Frogel, and Hwihyun Kim

Liu et al. 2013 The Astrophysical Journal Letters 778 L41.

  • Provider: AAS Journals

Caption: Figure 1.

[N ii]/Hα ratio map for M83 adopted in this work, overlaid on the Hα+[N ii] contour map. The letters and numbers denote the regions studied by Bresolin & Kennicutt (2002). Only the southern pointing is shown because none of the H ii regions in the northern pointing has been observed by those authors. The color bar to the right indicates the ratio of the total intensity of the nitrogen doublet (λλ6548, 6584 Å) to the Hα line intensity. The kinematic nucleus is marked with a white plus sign following Knapen et al. (2010), and the black dashed circles depict the galactic radii of 1, 2 and 3 kpc that are used for the calculations in Table 1 and Figure 3.

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