Time-dependent injection from bursty star formation or episodic black hole accretion substantially modifies cosmic ray pressure profiles in massive galaxy halos, flattening them at large radii relative to steady-state predictions.
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Time-Dependent Cosmic Ray Halos from Bursty Star Formation and Active Galactic Nuclei: Semi-Analytic Formalism and Galaxy Formation Implications
Time-dependent injection from bursty star formation or episodic black hole accretion substantially modifies cosmic ray pressure profiles in massive galaxy halos, flattening them at large radii relative to steady-state predictions.