Speaker: Yuki Takei

Title: A light curve model for type IIn supernovae

Type IIn supernovae (SNe IIn) exhibit narrow hydrogen emission lines in their spectra, which indicates the existence of dense circumstellar media (CSM). Ejecta collides with dense CSM and interaction between them occurs, making SNe IIn much more luminous than other normal SNe.
We construct a light curve model by resolving interaction region. In this talk I will present how to resolve the region.

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Last-modified: 2019-07-17 (水) 17:40:20 (3d)