Figure 3 from Explaining the Early Excess Emission of the Type Ia Supernova 2018oh by the Interaction of the Ejecta with Disk-originated Matter

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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 3.

Fitting an ejecta-DOM model to excess flux only. Here excess flux is total flux minus a L ∝ t² model for the contribution of the main nickel-heating light curve. Plot markings as in Figure 2.

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