Statements (56)
| Predicate | Object |
|---|---|
| gptkbp:instance_of |
gptkb:Ninjutsu
|
| gptkbp:can_create |
pulsed X-ray emissions
|
| gptkbp:characteristics |
rapid rotation
|
| gptkbp:discovered_by |
gptkb:1967
|
| gptkbp:emissions_standard |
gptkb:X-rays
radio waves |
| gptkbp:exhibits |
X-ray flares
periodic outbursts magnetar-like behavior spin-up and spin-down behavior timing noise |
| gptkbp:frequency |
pulsation period
|
| gptkbp:has |
strong magnetic field
|
| https://www.w3.org/2000/01/rdf-schema#label |
X-ray pulsar
|
| gptkbp:is_a |
gptkb:physicist
astrophysical phenomenon compact object high-energy astrophysical object source of gravitational waves type of neutron star |
| gptkbp:is_analyzed_in |
cosmological distances
matter under extreme conditions |
| gptkbp:is_associated_with |
gptkb:supernova_remnants
accretion processes accretion disks stellar collapse |
| gptkbp:is_characterized_by |
pulsation frequency
|
| gptkbp:is_found_in |
various galaxies
different types of galaxies |
| gptkbp:is_known_for |
strong gravitational fields
high-energy emissions emit bursts of radiation |
| gptkbp:is_observed_in |
various wavelengths
radio telescopes |
| gptkbp:is_often_depicted_as |
star clusters
|
| gptkbp:is_often_used_in |
astrophysical simulations
|
| gptkbp:is_part_of |
gptkb:the_Milky_Way
the universe pulsar timing arrays X-ray binary systems |
| gptkbp:is_related_to |
gamma-ray bursts
|
| gptkbp:is_studied_in |
X-ray spectroscopy
astrophysics stellar evolution magnetic field strength pulsar timing measurements |
| gptkbp:is_used_for |
studying extreme physics
|
| gptkbp:is_used_in |
gravitational wave detection
|
| gptkbp:located_in |
gptkb:star
|
| gptkbp:recognizes |
space telescopes
X-ray spectrum |
| gptkbp:scientific_classification |
soft or hard X-ray pulsar
type of X-ray source |
| gptkbp:bfsParent |
gptkb:X-ray_Binary
gptkb:Pulsar |
| gptkbp:bfsLayer |
3
|