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kilonova
EntityQ14468623· pop 28· linked from 212 articles

Also known as knova, macronova, r-process supernova, KN, kilonovae, KNe

thumb|upright=1.4|Artist's impression of neutron stars merging, producing gravitational waves and resulting in a kilonova

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Eso1733s Artist's impression of merging neutron stars.jpg
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Kilonovae
start time
2010-00-00
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  • History
  • Theory
  • Observations
  • See also
  • References
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thumb|upright=1.4|Artist's impression of neutron stars merging, producing gravitational waves and resulting in a kilonova

A kilonova (also called a macronova) is a transient astronomical event that occurs in a compact binary system when two neutron stars (BNS) or a neutron star and a black hole collide. The kilonova, visible over the weeks and months following the merger, is an isotropically expanding luminous afterglow of electromagnetic radiation emitted by the radioactive decay of r-process nuclei synthesized by—and then ejected from—the initial cataclysmic event.

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