gptkbp:instanceOf
|
astronomer
|
gptkbp:associatedWith
|
magnetars
|
gptkbp:burstDuration
|
milliseconds to seconds
|
gptkbp:burstEnergy
|
10^38–10^41 ergs
|
gptkbp:characterizedBy
|
repeated bursts of soft gamma rays
|
gptkbp:discoveredBy
|
Konus experiment
|
gptkbp:discoveredIn
|
1979
|
gptkbp:emits
|
gptkb:X-rays
gptkb:gamma_rays
|
gptkbp:example
|
gptkb:SGR_0526-66
gptkb:SGR_1627-41
gptkb:SGR_1806-20
gptkb:SGR_1900+14
|
gptkbp:foundIn
|
gptkb:Milky_Way
gptkb:Large_Magellanic_Cloud
|
https://www.w3.org/2000/01/rdf-schema#label
|
soft gamma repeaters
|
gptkbp:magneticFieldStrength
|
10^14–10^15 gauss
|
gptkbp:observedBy
|
gptkb:INTEGRAL_satellite
gptkb:Swift_Observatory
gptkb:Chandra_X-ray_Observatory
gptkb:Fermi_Gamma-ray_Space_Telescope
gptkb:XMM-Newton
RXTE satellite
|
gptkbp:powerSource
|
magnetic field decay
|
gptkbp:relatedTo
|
gptkb:gamma-ray_bursts
supernova remnants
pulsars
anomalous X-ray pulsars
|
gptkbp:rotationPeriod
|
2–12 seconds
|
gptkbp:subclassOf
|
white dwarf
|
gptkbp:bfsParent
|
gptkb:Konus-Wind
gptkb:Gamma-ray_Burst_Monitor
gptkb:Gamma-ray_Burst_Monitor_(GBM)
gptkb:MAXI
|
gptkbp:bfsLayer
|
7
|