Properties (50)
| Predicate | Object |
|---|---|
| gptkbp:instanceOf |
astronomical event
|
| gptkbp:associatedWith |
gravitational waves
short gamma-ray bursts |
| gptkbp:causedBy |
merger of neutron stars
|
| gptkbp:collaboratedWith |
international observatories
|
| gptkbp:collaborations |
multi-messenger astronomy
|
| gptkbp:contributedTo |
understanding of dark matter
|
| gptkbp:decidedBy |
theoretical astrophysics
|
| gptkbp:duration |
hours to days
|
| gptkbp:emissionsStandard |
electromagnetic radiation
|
| gptkbp:energyEfficiency |
nuclear reactions
10^51 ergs |
| gptkbp:established |
astronomers
|
| gptkbp:firstAwarded |
2017
|
| gptkbp:firstClaim |
nuclear astrophysics
future discoveries |
| gptkbp:hasRecognition |
UV to infrared
|
| gptkbp:historicalResearch |
ongoing studies
|
| https://www.w3.org/2000/01/rdf-schema#label |
Kilonovae
|
| gptkbp:iceClass |
can be detected in multiple wavelengths
|
| gptkbp:impact |
cosmology
|
| gptkbp:influencedBy |
stellar evolution
|
| gptkbp:influences |
galactic chemical evolution
|
| gptkbp:involvedIn |
modern astronomy
|
| gptkbp:length |
billions of light-years
|
| gptkbp:lighting |
fades over days to weeks
redder than supernovae |
| gptkbp:model |
r-process nucleosynthesis
|
| gptkbp:namedAfter |
kilo_(thousand)_nova_(new)
|
| gptkbp:occursAnnually |
rare events
|
| gptkbp:occursIn |
distant galaxies
|
| gptkbp:officialResidence |
telescopes
distance and faintness collected from various missions |
| gptkbp:produces |
heavy elements
|
| gptkbp:relatedEvent |
necessary for understanding
|
| gptkbp:relatedPatent |
supernovae
|
| gptkbp:relatedTo |
black hole formation
neutron_star_physics |
| gptkbp:researchField |
astrophysics
|
| gptkbp:researchInterest |
advances in technology
|
| gptkbp:scientificName |
understanding neutron star physics
|
| gptkbp:significance |
explains origin of gold and platinum
|
| gptkbp:thematicElement |
broad absorption lines
|
| gptkbp:theory |
merger dynamics
|
| gptkbp:visitedBy |
gptkb:Virgo
gptkb:LIGO gptkb:Hubble_Space_Telescope gamma-ray bursts Gravitational wave observatories |