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gptkbp:instance_of
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gptkb:Supernova
|
|
gptkbp:are_part_of
|
Astrophysical Research
|
|
gptkbp:are_the_end_state_of
|
gptkb:Massive_Stars
|
|
gptkbp:can
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gptkb:Accretion_Disks
Kilonova Events
Orbital Eccentricity
High Magnetic Fields
|
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gptkbp:can_be_found_in
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gptkb:Globular_Clusters
|
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gptkbp:can_cause
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gptkb:Gamma-Ray_Bursts
|
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gptkbp:can_collapse_into
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gptkb:Black_Holes
|
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gptkbp:can_create
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gptkb:Gravitational_Waves
Supernova Explosions
Heavy Elements
|
|
gptkbp:can_detect
|
gptkb:Electromagnetic_Radiation
Radio Telescopes
|
|
gptkbp:can_have_different
|
Masses
Spin Rates
|
|
gptkbp:can_have_magnetic_fields
|
up to 10^15 Gauss
|
|
gptkbp:can_have_temperature
|
up to 1 million K
|
|
gptkbp:composed_of
|
Neutrons
|
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gptkbp:emissions_standard
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gptkb:X-rays
|
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gptkbp:example
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gptkb:Compact_Objects
|
|
gptkbp:exhibits
|
Gravitational Redshift
Relativistic Effects
Tidal Forces
Gravitational Lensing
Pulsar Behavior
Magnetar Activity
Spin-Down
|
|
gptkbp:formed
|
gptkb:Massive_Stars
|
|
gptkbp:has_a_focus_on
|
Astrophysical Simulations
Gravitational Wave Astronomy
Astrophysical Research Programs
Observational Campaigns
|
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gptkbp:has_radius
|
about 10 km
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Two Neutron Stars
|
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gptkbp:is_a_source_of
|
gptkb:Short_Gamma-Ray_Bursts
Electromagnetic Counterparts
Neutrino Emission
|
|
gptkbp:is_a_subject_of
|
Theoretical Research
|
|
gptkbp:is_considered
|
gptkb:cosmology
Nuclear Astrophysics
High-Energy Astrophysics
Extreme States of Matter
|
|
gptkbp:is_essential_for
|
Understanding Gravity
|
|
gptkbp:is_found_in
|
Binary Systems
|
|
gptkbp:is_involved_in
|
Astrophysical Phenomena
|
|
gptkbp:is_located_in
|
Galaxies
|
|
gptkbp:is_observed_in
|
Various Wavelengths
|
|
gptkbp:is_part_of
|
gptkb:Supernova_Remnants
Astrophysical Models
Astrophysical Observations
Gravitational Wave Events
|
|
gptkbp:is_related_to
|
gptkb:Neutron_Star_Mergers
|
|
gptkbp:is_studied_for
|
Nuclear Physics
Astrophysical Implications
Neutron Star Physics
Equation of State
|
|
gptkbp:is_studied_in
|
gptkb:astronomy
Multi-Messenger Astronomy
|
|
gptkbp:is_tested_for
|
gptkb:General_Relativity
|
|
gptkbp:mass
|
1.4 to 2.16 solar masses
|
|
gptkbp:merged_with
|
gptkb:Yes
|
|
gptkbp:orbital_period
|
milliseconds to hours
|
|
gptkbp:population_density
|
about 4 x 10^17 kg/m^3
|
|
gptkbp:was_a_result_of
|
gptkb:Core-Collapse_Supernovae
Stellar Evolution
Binary Star Evolution
Stellar Collapse
|
|
gptkbp:bfsParent
|
gptkb:Neutron_Star_Binary
gptkb:Neutron_Star_Mergers
|
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gptkbp:bfsLayer
|
5
|