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Detection and Evolution of Linear Polarization of the Galactic Center Transient MAXI J1744-294

  • Authors: Joseph M. Michail, Sebastiano D. von Fellenberg, Mayura Balakrishnan, Geoffrey C. Bower, Nicole M. Ford, Zach Sumners, Giovanni G. Fazio, Daryl Haggard, Joseph L. Hora, Garrett K. Keating, J. D. Livingston, Sera Markoff, Bart Ripperda, Sophia Sánchez-Maes, Howard A. Smith, S. P. Willner, Jun-Hui Zhao

Joseph M. Michail et al 2026 The Astrophysical Journal 1003 .

  • Provider: AAS Journals

Caption: Figure 3.

Normalized Stokes q and u parameters of MAXI J1744 on the 2025 April 6 epoch compared with the best-fit m1 (dashed light green lines; single component) and m11 (solid black lines; double component) models. Appendix D gives more details about the models. Left: Stokes q and u spectra. Right: Stokes q vs. u plot. The data point colors correspond to the observing frequency, matching the color scheme in Figure 1.

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