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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 5.

Line ratios comparing different ionization states of argon ([Ar II] 15.8 eV and [Ar III] 27.6 eV), sulfur ([S III] 23.3 eV and [S IV] 34.8 eV), and neon ([Ne II] 21.6 eV and [Ne III] 40.96 eV). Ratios are calculated for the Bar (maroon), Northern Arm (orange), and BC structures (yellow) in the spatial apertures labeled Region 1 (circles), Region 2 (squares), and Region 3 (triangles). The line of best fit and 1σ confidence band are shown in gray. Arrows indicate 3σ limits (due to either [Ne II] saturation or [S III] nondetection). The BC structures are more ionized than the Northern Arm, which is more ionized than the Bar; Regions 1 and 2 are always more ionized than Region 3.

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