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First Mid-infrared Detection and Modeling of a Flare from Sgr A*

  • Authors: Sebastiano D. von Fellenberg, Tamojeet Roychowdhury, Joseph M. Michail, Zach Sumners, Grace Sanger-Johnson, Giovanni G. Fazio, Daryl Haggard, Joseph L. Hora, Alexander Philippov, Bart Ripperda, Howard A. Smith, S. P. Willner, Gunther Witzel, Shuo Zhang, Eric E. Becklin, Geoffrey C. Bower, Sunil Chandra, Tuan Do, Macarena Garcia Marin, Mark A. Gurwell, Nicole M. Ford, Kazuhiro Hada, Sera Markoff, Mark R. Morris, Joey Neilsen, Nadeen B. Sabha, Braden Seefeldt-Gail

Sebastiano D. von Fellenberg et al 2025 The Astrophysical Journal Letters 979 .

  • Provider: AAS Journals

Caption: Figure 1.

MIR images of the Galactic center with JWST. The color insets show JWST 5.3 μm (A), 8.1 μm (B), 12.5 μm (C), and 19.3 μm (D) observations. The JWST/MIRI images are superposed on the ﹩L^{\prime} ﹩ (NIR 3.8 μm) stellar-background image from the Keck Observatory (J. L. Hora et al. 2014). The image scale is labeled in arcseconds with Sgr A* at the origin. North is up, east to the left.

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