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X-Ray Light Curve and Spectra of Shock Breakout in a Wind

  • Authors: Yukari Ohtani, Akihiro Suzuki, Toshikazu Shigeyama, and Masaomi Tanaka

2018 The Astrophysical Journal 853 52.

  • Provider: AAS Journals

Caption: Figure 3.

Light curve (0.3–10 keV) of emission originating from a spherically symmetric shock. The superposed bars are the observed data of XRO 080109. The time is measured from the moment when the first photon passes a large spherical surface concentric with the ejecta.

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