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Discrete and Continuous Ejection Models of the Radio Source Associated with GW170817

  • Authors: Brian Punsly

2019 The Astrophysical Journal Letters 871 L34.

  • Provider: AAS Journals

Caption: Figure 5.

Other constraints on the models. The top panel compares the decay from the peak of the 3 GHz light curve in the models to that of the least squares fit to the data. The bottom panel shows that radiative losses are too large for the discrete ejection model unless Γmin = 1. The maximum and minimum conditions are described in the text.

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