Gamma-ray burst outflows may entrain small blobs or filaments of dense, highly ionized metal-rich material. Such inhomogeneities, accelerated by the flow to Lorentz factors in the range 10-100, could have a significant coverage factor and give rise to broad features, especially because of Fe K edges, which influence the spectrum below the MeV range, leading to a progressively decreasing hardness ratio.
CITATION STYLE
Mészáros, P., & Rees, M. J. (1998). Spectral Features from Ultrarelativistic Ions in Gamma-Ray Bursts? The Astrophysical Journal, 502(2), L105–L108. https://doi.org/10.1086/311499
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