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gptkbp:instance_of
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gptkb:physicist
|
|
gptkbp:bfsLayer
|
3
|
|
gptkbp:bfsParent
|
gptkb:Neutron_Star_Crust
|
|
gptkbp:average_temperature
|
Millions of Kelvin
|
|
gptkbp:consists_of
|
Neutron Degenerate Matter
|
|
gptkbp:demands
|
Tremendous Pressure
|
|
gptkbp:dissolved
|
gptkb:football_club
|
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gptkbp:emissions_standard
|
gptkb:X-rays
|
|
gptkbp:examines
|
gptkb:spacecraft
Stellar Dynamics
Astrophysical Simulations
|
|
gptkbp:exhibits
|
gptkb:Gravitational_Waves
|
|
gptkbp:financial_performance
|
Neutron Degeneracy Pressure
|
|
gptkbp:formed
|
Supernova Explosion
|
|
https://www.w3.org/2000/01/rdf-schema#label
|
Outer Layer of Neutron Star
|
|
gptkbp:is_affected_by
|
Thermal Conductivity
Neutrino Emission
Magneto-hydrodynamics
|
|
gptkbp:is_associated_with
|
gptkb:Magnetars
Thermal Emission
X-ray Binaries
|
|
gptkbp:is_characterized_by
|
High Density
Rapid Rotation
High Rotation Rates
High Magnetic Fields
|
|
gptkbp:is_connected_to
|
gptkb:Neutron_Star_Crust
gptkb:Superfluidity
Pulsar Timing
Neutron Star Oscillations
|
|
gptkbp:is_considered
|
Theoretical Models of Stellar Evolution
|
|
gptkbp:is_critical_for
|
Astrophysical Observations
|
|
gptkbp:is_described_as
|
gptkb:political_movement
Relativistic Effects
Equation of State
|
|
gptkbp:is_influenced_by
|
gptkb:Electromagnetic_Radiation
Magnetic Fields
Tidal Forces
|
|
gptkbp:is_involved_in
|
gptkb:Neutron_Star_Mergers
gptkb:Gamma-ray_Bursts
Astrophysical Observations
Pulsar Emission
|
|
gptkbp:is_linked_to
|
gptkb:Neutron_Star_Crust
Nuclear Physics
Astrophysical Jets
|
|
gptkbp:is_observed_in
|
gptkb:observatory
|
|
gptkbp:is_part_of
|
gptkb:physicist
gptkb:Compact_Objects
Astrophysical Phenomena
Stellar Remnants
Neutron Star Structure
Neutron Star Evolution
|
|
gptkbp:is_related_to
|
gptkb:political_movement
|
|
gptkbp:is_studied_in
|
Gravitational Collapse
Astrophysical Research
Astrophysical Models
Understanding of Matter Under Extreme Conditions
|
|
gptkbp:is_subject_to
|
Nuclear Reactions
Extreme Gravity
|
|
gptkbp:located_in
|
Core of Neutron Star
|
|
gptkbp:population
|
About 4 x 10^17 kg/m^3
|