young pulsar

GPTKB entity

Statements (67)
Predicate Object
gptkbp:instance_of gptkb:Ninjutsu
gptkbp:bfsLayer 3
gptkbp:bfsParent gptkb:Pulsar
gptkbp:age less than 1 million years
gptkbp:can_be strong gravitational fields
accretion disks
high surface temperatures
high rotational energy
gptkbp:emissions_standard gptkb:X-rays
gamma rays
pulsed radiation
gptkbp:exhibits precession
glitches
timing irregularities
magnetar-like behavior
gptkbp:field gptkb:theorem
gptkbp:focuses_on observational campaigns
gptkbp:formed gptkb:core-collapse_supernovae
gptkbp:has_gameplay_element high-energy astrophysics
gptkbp:has_lore gptkb:theorem
gptkbp:has_spectral_type radio waves
gptkbp:has_spin_off hundreds of times per second
https://www.w3.org/2000/01/rdf-schema#label young pulsar
gptkbp:is_a_source_of pulsar wind nebulae
pulsar glitches
gptkbp:is_analyzed_in gptkb:observatory
dark matter interactions
gptkbp:is_associated_with gptkb:physicist
high-energy particles
gamma-ray bursts
pulsar timing arrays
pulsar timing measurements
gptkbp:is_atype_of gptkb:star
compact star
astrophysical object
exotic star
neutron star binary
gptkbp:is_considered a laboratory for physics
gptkbp:is_found_in gptkb:the_Crab_Nebula
gptkb:supernova_remnants
gptkb:the_Large_Magellanic_Cloud
globular clusters
gptkbp:is_known_for its rapid rotation
gptkbp:is_observed_in X-ray wavelengths
gptkbp:is_often_compared_to old pulsars
gptkbp:is_often_depicted_as binary systems
gptkbp:is_often_used_in astrophysical simulations
gptkbp:is_part_of gptkb:the_Milky_Way
stellar evolution studies
theoretical models of neutron stars
the study of cosmic evolution
the search for gravitational waves
pulsar population studies
gptkbp:is_studied_in astrophysics
gravity
stellar magnetic fields
nuclear physics applications
cosmic ray origins
its emission mechanisms
its magnetic field structure
stellar collapse mechanisms
gptkbp:is_tested_for theories of relativity
quantum gravity theories
gptkbp:may_have gptkb:theorem
gptkbp:recognizes space telescopes
radio telescopes
gptkbp:research neutron star equations of state