AT 2017gfo
E1846251
UNEXPLORED
AT 2017gfo is the kilonova optical/infrared transient associated with the first observed binary neutron star merger, providing key evidence for heavy element production via r-process nucleosynthesis.
All labels observed (1)
| Label | Occurrences |
|---|---|
| AT 2017gfo canonical | 1 |
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.