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JWST Observations of Starbursts: Polycyclic Aromatic Hydrocarbons Closely Trace the Cool Phase of M82’s Galactic Wind

  • Authors: Sebastian Lopez, Colton Ring, Adam K. Leroy, Serena A. Cronin, Alberto D. Bolatto, Laura A. Lopez, Vicente Villanueva, Deanne B. Fisher, Todd A. Thompson, Grant P. Donnelly, Lee Armus, Torsten Böker, Leindert A. Boogaard, Martha L. Boyer, Ryan Chown, Daniel A. Dale, Keaton Donaghue, Kimberly Emig, Simon C. O. Glover, Rodrigo Herrera-Camus, Ralf S. Klessen, Thomas S.-Y. Lai, Laura Lenkić, Rebecca C. Levy, David S. Meier, Elisabeth Mills, Juergen Ott, Evan D. Skillman, J. D. T. Smith, Elizabeth J. Tarantino, Sylvain Veilleux, Fabian Walter, Paul P. van der Werf

Sebastian Lopez et al 2026 The Astrophysical Journal Letters 999 .

  • Provider: AAS Journals

Caption: Figure A1.

Residual plots showing gas phase intensity (y-axis) and F770W intensity (x-axis) corrected for distance. From left to right, the columns are for CO(1–0), Hα, and X-ray. From top to bottom, the rows are distance separations at 0–1.05 kpc, 1.05–2.11 kpc, and 2.11–3.16 kpc. The upper distance bound is the maximum distance from all datasets. The black points are the medians for the distribution of data points, and the error bars are the 16th and 84th percentiles. In the top left of each panel, we show the best power-law fits to the medians and Spearman's rank correlation coefficient of the whole distribution.

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