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Persistent X-Ray Emission from ASASSN-15lh: Massive Ejecta and Pre-SLSN Dense Wind?

  • Authors: Yan Huang and Zhuo Li

2018 The Astrophysical Journal 859 123.

  • Provider: AAS Journals

Caption: Figure 3.

Model synchrotron spectrum in comparison with the radio limits from observations. The thick (thin) lines represent synchrotron flux with (without) free–free absorption taken into account. Three cases satisfying X-ray constraints are as marked as black solid points in Figure 2, ﹩({A}_{38},{\beta }_{0,-2})=(0.6,3)﹩ (red solid lines), (1.0, 1.9) (black dashed lines), and (1.2, 1.5) (blue dotted lines). The other parameters used are ﹩{\epsilon }_{B}=0.1﹩, ﹩{\epsilon }_{{\rm{e}}}=0.1﹩, p = 3, and ﹩{T}_{{\rm{e}}}=2.0\times {10}^{4}\,{\rm{K}}﹩.

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