A Global Photoionization Response to Prompt Emission and Outliers: Different Origin of Long Gamma-ray Bursts?
J. Wang, L. P. Xin, Y. L. Qiu, D. W. Xu, J. Y. Wei

TL;DR
This study investigates how the ionization state of the interstellar medium around long gamma-ray bursts correlates with their prompt emission properties, revealing potential different origins for outliers and typical bursts.
Contribution
It introduces a global photoionization response model linking ISM ionization ratios to gamma-ray burst prompt emission parameters, suggesting different progenitors for outliers.
Findings
Ionization ratio increases with $L_{iso}/E_{peak}$ and $L_{iso}/E_{peak}^2$ for most LGRBs.
Outliers show high ionization ratios and Wolf-Rayet star signatures.
Scatter in the Amati relation may be related to ISM ionization states.
Abstract
By using the line ratio \ion{C}{4}/\ion{C}{2} as a tracer of ionization ratio of the interstellar medium (ISM) illuminated by a long gamma-ray burst (LGRB), we identify a global photoionization response of the ionization ratio to the photon luminosity of the prompt emission assessed by either or . The ionization ratio increases with both and for a majority of the LGRBs in our sample, although there are a few outliers. The identified dependence of \ion{C}{4}/\ion{C}{2} on suggests that the scatter of the widely accepted Amati relation is related with the ionization ratio in ISM. The outliers tend to have relatively high \ion{C}{4}/\ion{C}{2} values as well as relatively high…
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