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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 2.

The distribution of MUSE IFU data for NGC 5728 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). An interactive version of this figure is available in the online journal.

An interactive version of this figure is available in the online article.

An interactive version of this figure is available.

An interactive version of this figure is available in the online journal.

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