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Ionization Structure and Metal Enrichment of the Galactic Center Minispiral Observed with JWST

  • Authors: Nicole M. Ford, Mayura Balakrishnan, Sebastiano D. von Fellenberg, Daryl Haggard, Joseph M. Michail, Yuzhu Cui, Joseph L. Hora, Joey Neilsen, Giacomo Principe, Tamojeet Roychowdhury, Nadeen B. Sabha, Howard A. Smith, Zach Sumners, S. P. Willner

Nicole M. Ford et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 1.

The Galactic Minispiral as seen in the mid-infrared (MIR). The panels zoom in from left to right. Left: the VISIR PAH1 8.58 μm image (C. K. Dinh et al. 2024), middle: MIRI Medium Resolution Spectrograph (MRS) summed flux in spectral channel 4 (Ch4; 17.70–27.90 μm), and right: spectral channel 1 (Ch1; 4.9–7.65 μm). The left panel is overlaid with coordinates colored by gas radial velocity derived from Brγ (M. S. Nitschai et al. 2020). Sgr A*’s position is marked with a white star in all panels. In the middle and right panels, W-R star positions (T. Paumard et al. 2006; A. Ciurlo et al. 2023; C. K. Dinh et al. 2024) are marked with gray crosses, and a selection of compact structures (C. K. Dinh et al. 2024) are marked with gray circles. Spectral extraction apertures are labeled with black circles.

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