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- W2892216909 abstract "We extend our study of energetic radio loud and quiet gamma-ray bursts (GRBs), suggesting these GRBs potentially come from two separate progenitor systems. We expand the sample from our previous paper (Lloyd-Ronning & Fryer, 2017) and find our results are strengthened - radio quiet GRBs have significantly shorter intrinsic prompt duration, and are also less energetic on average. However, the tenuous correlation between isotropic energy and intrinsic duration in the radio dark sample remains tenuous and is slightly weakened by adding more bursts. Interestingly, we find an anti-correlation between the intrinsic duration and redshift in the radio bright sample but not the radio dark sample, further supporting that these two samples may come from separate progenitors. We also find that very high energy (0.1 - 100 GeV) extended emission is only present in the radio loud sample. There is no significant difference between the presence of X-ray plateaus or the average jet opening angles between the two samples. We explore the interpretation of these results in the context of different progenitor models. The data are consistent with the radio loud GRBs coming from a Helium-merger system and the radio quiet GRBs coming from a collapsar system." @default.
- W2892216909 created "2018-09-27" @default.
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- W2892216909 date "2018-09-11" @default.
- W2892216909 modified "2023-10-16" @default.
- W2892216909 title "Cosmological Evolution of the Intrinsic Prompt Duration for Radio Bright Gamma-Ray Bursts" @default.
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