Radiative-transfer models for dusty Type II supernovae

Open Access

Fig. 7.

Extinction due to ejecta dust for the SN IIn model. We consider dust masses between 10⁻⁶ and 10⁻³ M_⊙ and show the results for the UVW1-band (ultraviolet range) and V-band filters. As in Fig. 6, the dust is placed in the outer-ejecta dense shell. [see Sect. 5 for discussion.]

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