KnowraPulsarLinked fromLinked fromThe 42 pages that link to Pulsar, each with the reason it gives.All 42Broader topic 13Related 15Narrower topic 10Compared with 4Gamma rayRelated: Some pulsars emit periodic gamma rays powered by particle acceleration in their magnetospheres.Gamma-ray astronomyRelated: Gamma-ray observations reveal energetic pulsars and help locate where their magnetospheres accelerate particles.Arecibo ObservatoryRelated: Arecibo observations helped establish the nature of the first binary pulsar.Circular polarizationRelated: Pulsar radio signals can contain measurable circular polarization that reveals magnetized emission conditions.Faraday rotationRelated: Pulsar polarization and dispersion measurements constrain magnetic fields in intervening plasma.PrecessionRelated: Precession can alter a pulsar's beam direction and produce long-term changes in its observed pulses.National Radio Astronomy ObservatoryRelated: Radio observatories such as NRAO's facilities made pulsar timing and population studies possible.Fermi Gamma-ray Space TelescopeRelated: Fermi's gamma-ray survey revealed many pulsars, including ones faint at radio wavelengths.Green Bank TelescopeRelated: The telescope’s sensitivity supports precise timing and searches for faint pulsars.Martin RyleRelated: The 1974 Nobel citation also recognized Hewish’s role in discovering pulsars.Quark starRelated: Some pulsars have measured masses and timing properties that constrain compact-star models.Jodrell Bank ObservatoryRelated: Pulsar observations became a major research program at the observatory.Five-hundred-meter Aperture Spherical TelescopeRelated: FAST has discovered many pulsars by detecting their faint periodic radio signals.Effelsberg 100-metre Radio TelescopeRelated: Effelsberg’s sensitive observations have helped measure pulsar signals and their timing.Low-Frequency ArrayRelated: LOFAR's low-frequency sensitivity supports studies of pulsar emission and propagation through space.
KnowraPulsarLinked fromLinked fromThe 42 pages that link to Pulsar, each with the reason it gives.All 42Broader topic 13Related 15Narrower topic 10Compared with 4Gamma rayRelated: Some pulsars emit periodic gamma rays powered by particle acceleration in their magnetospheres.Gamma-ray astronomyRelated: Gamma-ray observations reveal energetic pulsars and help locate where their magnetospheres accelerate particles.Arecibo ObservatoryRelated: Arecibo observations helped establish the nature of the first binary pulsar.Circular polarizationRelated: Pulsar radio signals can contain measurable circular polarization that reveals magnetized emission conditions.Faraday rotationRelated: Pulsar polarization and dispersion measurements constrain magnetic fields in intervening plasma.PrecessionRelated: Precession can alter a pulsar's beam direction and produce long-term changes in its observed pulses.National Radio Astronomy ObservatoryRelated: Radio observatories such as NRAO's facilities made pulsar timing and population studies possible.Fermi Gamma-ray Space TelescopeRelated: Fermi's gamma-ray survey revealed many pulsars, including ones faint at radio wavelengths.Green Bank TelescopeRelated: The telescope’s sensitivity supports precise timing and searches for faint pulsars.Martin RyleRelated: The 1974 Nobel citation also recognized Hewish’s role in discovering pulsars.Quark starRelated: Some pulsars have measured masses and timing properties that constrain compact-star models.Jodrell Bank ObservatoryRelated: Pulsar observations became a major research program at the observatory.Five-hundred-meter Aperture Spherical TelescopeRelated: FAST has discovered many pulsars by detecting their faint periodic radio signals.Effelsberg 100-metre Radio TelescopeRelated: Effelsberg’s sensitive observations have helped measure pulsar signals and their timing.Low-Frequency ArrayRelated: LOFAR's low-frequency sensitivity supports studies of pulsar emission and propagation through space.