Two Neutron Stars

GPTKB entity

Statements (72)
Predicate Object
gptkbp:instance_of gptkb:physicist
gptkbp:bfsLayer 3
gptkbp:bfsParent gptkb:Neutron_Star_Binary
gptkb:Neutron_Star_Mergers
gptkbp:can_be gptkb:Accretion_Disks
Kilonova Events
Orbital Eccentricity
High Magnetic Fields
gptkbp:can_create gptkb:battle
gptkb:Gravitational_Waves
Masses
Supernova Explosions
Heavy Elements
Spin Rates
gptkbp:caused_by gptkb:Gamma-Ray_Bursts
gptkbp:composed_of Neutrons
gptkbp:diameter about 10 km
gptkbp:dissolved gptkb:Black_Holes
gptkbp:emissions_standard gptkb:X-rays
gptkbp:ends_at gptkb:Massive_Stars
gptkbp:example gptkb:Compact_Objects
gptkbp:exhibits Gravitational Redshift
Relativistic Effects
Tidal Forces
Gravitational Lensing
Pulsar Behavior
Magnetar Activity
Spin-Down
gptkbp:field up to 10^15 Gauss
gptkbp:focuses_on Astrophysical Simulations
Gravitational Wave Astronomy
Astrophysical Research Programs
Observational Campaigns
gptkbp:formed gptkb:Massive_Stars
https://www.w3.org/2000/01/rdf-schema#label Two Neutron Stars
gptkbp:is_a_source_of gptkb:Short_Gamma-Ray_Bursts
Electromagnetic Counterparts
Neutrino Emission
gptkbp:is_considered gptkb:spacecraft
Nuclear Astrophysics
High-Energy Astrophysics
Extreme States of Matter
gptkbp:is_essential_for Understanding Gravity
gptkbp:is_found_in gptkb:Globular_Clusters
Binary Systems
gptkbp:is_involved_in Astrophysical Phenomena
gptkbp:is_observed_in Various Wavelengths
gptkbp:is_part_of gptkb:Supernova_Remnants
Astrophysical Research
Astrophysical Models
Astrophysical Observations
Gravitational Wave Events
gptkbp:is_related_to gptkb:Neutron_Star_Mergers
gptkbp:is_studied_in gptkb:observatory
Nuclear Physics
Multi-Messenger Astronomy
Astrophysical Implications
Neutron Star Physics
Equation of State
gptkbp:is_tested_for gptkb:General_Relativity
gptkbp:located_in Galaxies
gptkbp:mass 1.4 to 2.16 solar masses
gptkbp:orbital_period milliseconds to hours
gptkbp:population about 4 x 10^17 kg/m^3
gptkbp:recognizes gptkb:Electromagnetic_Radiation
Radio Telescopes
gptkbp:result gptkb:Core-Collapse_Supernovae
Stellar Evolution
Binary Star Evolution
Stellar Collapse
gptkbp:serving_temperature up to 1 million K
gptkbp:subject Theoretical Research