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Explaining the Early Excess Emission of the Type Ia Supernova 2018oh by the Interaction of the Ejecta with Disk-originated Matter

  • Authors: Naveh Levanon, and Noam Soker

2019 The Astrophysical Journal Letters 872 L7.

  • Provider: AAS Journals

Caption: Figure 1.

Schematic drawing of the flow structure just after explosion. The blue regions represent the DOM, which has both a partial axial symmetry and a mirror symmetry. Here the two hemispheres present two cases. The upper half presents a general DOM structure and the lower half presents the two-component toy model described in Section 3.

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