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A Theoretical Three-dimensional Diagram to Separate Star Formation, Active Galactic Nuclei, and Shocks in Galaxies

  • Authors: Peixin Zhu, Lisa J. Kewley, Ralph S. Sutherland, Kathryn Grasha

Peixin Zhu et al 2025 The Astrophysical Journal 988 .

  • Provider: AAS Journals

Caption: Figure 5.

The distribution of WiFeS IFU data for NGC 5728 (observed in the S7 survey) on the new theoretical 3D diagram, with the spaxels color-coded by H II contribution fraction (top left), AGN contribution fraction (top right), fast-shock contribution fraction (bottom left), and pure-shock contribution fraction (bottom right).

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