i Register
In some senses, kilonova is marked as informal. Watch for register when choosing this word.
ADJ.
due, near-infrared, optical
VERB + KILONOVA
bump, shine
PREP.
in
ADV.
also
noun
A type of supernova that is underluminous, caused by the merger of two neutron stars
A radiation pattern typical of a kilonova.
Moreover, during merger neutron-rich matter can be ejected that can shine as a kilonova due to the decay of r-process elements [2–13].
The observed energetics and temporal/spectral properties of the late infrared bump (ie, the "kilonova") are also found to be consistent with emission from the ejecta launched during a neutron star (NS)-NS merger and powered by a magnetar central engine.
Moreover, during merger neutron-rich matter can be ejected that can shine as a kilonova due to the decay of r-process elements [2–13].
WiktionaryThe observed energetics and temporal/spectral properties of the late infrared bump (ie, the "kilonova") are also found to be consistent with emission from the ejecta launched during a neutron star (NS
WiktionaryDisk winds generally contribute to a ~week long transient peaking in the near-infrared (kilonova), although an optical precursor can manifest as a signature of delayed black hole formation or high bla
Wiktionaryi Register
In some senses, kilonova is marked as informal. Watch for register when choosing this word.