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The Spatially Resolved Hot Gas Properties of NGC 1266’s Active Galactic Nucleus-driven Outflow

  • Authors: Sebastian Lopez, Laura A. Lopez, Lauranne Lanz, Justin A. Otter, Katherine Alatalo

Sebastian Lopez et al 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 7.

First and second: gradients with distance of the median ne and P/k values from the MUSE data. Third and fourth: ratio plots comparing the ne and P/k values from MUSE and our X-ray spectral analysis. We find that the warm and hot outflow phases reach near pressure equilibrium at the outflow's maximum extent.

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