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Infrared Line Diagnostics Fail to Constrain Sgr A*’s UV Output

  • Authors: Mayura Balakrishnan, Sebastiano D. von Fellenberg, Daryl Haggard, Joseph M. Michail, Nicole M. Ford, Joseph L. Hora, Laurent Loinard, Sera Markoff, Joey Neilsen, Giacomo Principe, Nadeen B. Sabha, Howard A. Smith, Zach Sumners, Shuo Zhang

Mayura Balakrishnan et al 2026 The Astrophysical Journal 1008 .

  • Provider: AAS Journals

Caption: Figure 1.

JWST/MIRI Channel 1 5.6 micron image of the Galactic center field. Prominent sources are labeled in black. The position of Sgr A⋆ is marked by the yellow “X,” and the white circle indicates the 0﹩\mathop{.}\limits^{^{\prime\prime} }﹩3 radius aperture used for spectral extraction. The color scale shows the calibrated surface brightness in units of MJy sr−1.

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