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The Three-Dimensional Dynamic Structure of the Inner Orion Nebula

  • Authors: C. R. O'Dell, W. J. Henney, N. P. Abel, G. J. Ferland, and S. J. Arthur

O'DELL et al. 2009 The Astronomical Journal 137 367.

  • Provider: AAS Journals

Caption: Figure 7.

Physical structure for our constant-pressure model of the ionized, atomic, and molecular gas in the Orion-S Cloud. Plotted as a function of depth into the model are the (a) density, (b) gas and dust temperatures (c), molecular abundances, and (d) pressure constituents.

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