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An energetic dirty fireball detected in soft X-rays

Published 27 Mar 2026 in astro-ph.HE | (2603.26213v1)

Abstract: The collapse of massive stars drives explosions that power relativistic fireballs. If only a small amount of matter is entrained, such clean fireballs can expand with Lorentz factors $Γ&gt; 100$, accounting for gamma-ray bursts (GRBs). It has been hypothesized that energetic explosions with more baryon contamination, dubbed ``dirty fireballs'', may exist in nature, but they have not been observed. Here we report the observation of an extragalactic fast X-ray transient, EP241113a, detected by Einstein Probe. Compared to GRBs, it has a similar isotropic energy of 1.4×10<sup>511.4\times 10<sup>{51} erg, but significantly lower spectral peak energy. Theoretical modeling of its early X-ray afterglow suggests a relativistic jet with a low Lorentz factor of Γ20Γ\sim 20 aligned close to the line-of-sight, signifying the prototype of a dirty fireball.

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