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Table of Contents
Kilonovae
Kilonovae are electromagnetic transients observable in the infrared, optical, and ultraviolet bands. They originate from the neutron-rich outflows that are created during and after the merger of a binary neutron star or black hole – neutron star systems.
Heavy-element production
Radiative-Transfer Simulations
Last modified: le 2022/02/07 22:31
