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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 1.

Left: log-stretched JWST F770W image of M82 with dust and stellar continuum and background subtracted, capturing the strength of the 7.7 μm PAH feature. Blank pixels in the center are where the detector is saturated. Right: same as left, but for the F1130W data tracing the 11.3 μm PAH feature. In the top right, the PSF of the final images is shown.

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