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DOE OSTI · 2346046

Light Curves and Spectra from Kilonova Models [Poster]

Wollaeger, Ryan Thomas
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Abstract

White dwarf-neutron star merger simulations show a Ca IR line feature in spectra, pointing to Ca-rich transients as a possible observation (Kaltenborn et al 2024, Gillanders et al 2024). Supernova and new/old kilonova (KN) models have been compared to recent peculiar long gamma-ray burst (GRB) with KN-like signal (Troja et al 2022).

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BibTeXRIS

Wollaeger, Ryan Thomas. 2024-05-02. Light Curves and Spectra from Kilonova Models [Poster]. https://doi.org/10.2172/2346046

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