Physical Conditions of the Ionized Superwind in NGC 253 with VLT/MUSE
Published in ApJ, 2025
What is the physical state of ionized gas in galactic winds? In NGC 253, a prototypical starburst with a galactic wind, we found that the ionized gas is approaching speeds of 500 km/s, dominated by shock ionization, and is the product of a mere 2% starburst efficiency. This was my first project in graduate school, and culminated in the equivalent of my Master’s thesis.
Recommended citation: Cronin, S.A., et al. (2025), ApJ, 987, 92
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