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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 1.

Schematic view of an ellipsoidal shock propagating into a steady, spherically symmetric CSM. The degree of the shock asphericity is characterized by the oblateness f. The position of the shock front corresponds to the dashed curve at the moment of breakout.

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