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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 C2.

Distribution of model magnetic field values as β and Ti/Te are varied. The green line shows all parameter combinations that result in a 45 G magnetic field, while the red cross indicates EHT's magnetic field value for their chosen parameters of β = 1 and Ti/Te = 3.

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