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Galaxy Emission Line Classification Using Three-dimensional Line Ratio Diagrams

  • Authors: Frédéric P. A. Vogt, Michael A. Dopita, Lisa J. Kewley, Ralph S. Sutherland, Julia Scharwächter, Hassan M. Basurah, Alaa Ali, and Morsi A. Amer

Vogt et al. 2014 The Astrophysical Journal 793 127.

  • Provider: AAS Journals

Caption: Figure 1.

Example of a 3D line ratio diagram, labeled (a.k.a. log [N II]/[O II] versus log [O III]/[S II] versus log [N II]/Hα), in the form of a cross-eyed stereo pair. The plane of MAPPINGS IV simulations of H II regions is represented by the colored spheres connected by the gray rods, where each sphere corresponds to one distinct simulation. The color indicates the oxygen abundance in terms of 12 + log (O/H). Individual cubes correspond to the van Zee et al. (1998) data points, and the small cones to the NCG 5472 measurements of individual H II regions, also colored as a function of their metallicity. Detailed instructions to view this cross-eyed stereo pair can be found in Vogt & Wagner (2012). An .HTML file containing an interactive version of this Figure is available as supplementary material, and can also be directly accessed online (http://dx.doi.org/10.1088/0004-637X/793/2/127/data).

(A color version and supplemental data of this figure are available in the online journal.)

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