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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 1.

The top-left (top-right) frame is the radio data from epoch 1 (epoch 2). The SSA power-law fits of Equation (5) are the continuous curves (see Sections 2 and 3). The bottom frames extrapolate the power-law fit above 3 GHz to lower frequency revealing an excess at 675 MHz. The data in this figure is from Margutti et al. (2018), Troja et al (2018a), and Resmi et al (2018).

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