RRATs number up to 400000 in the Galaxy with a birth rate of at most 1.4 per century, comparable in size to pulsars at high luminosities and consistent with supernova rates.
@doi [ ] 10.1086/501516, https://ui.adsabs.harvard.edu/abs/2006ApJ...643..332F 643
4 Pith papers cite this work. Polarity classification is still indexing.
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TeV-selected PWNe and unidentified sources yield beaming fractions of 0.1-0.3 across radio, gamma-ray, and X-ray bands, with survey-to-survey differences explained by selection biases or older pulsars and reproducible via time-dependent opening angles.
Population synthesis of pulsar-massive star binaries yields an estimate for the number of observable VHE gamma-ray sources in the Galaxy, incorporating anisotropic wind-interaction zones.
The routine model with bulk viscosity best reproduces the Crab pulsar's magnetic inclination angle, spin period, and derivative, while electromagnetic torque and accretion suppress inclination growth and most other effects are negligible.
citing papers explorer
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The RRATalog: a Galactic census of rotating radio transients
RRATs number up to 400000 in the Galaxy with a birth rate of at most 1.4 per century, comparable in size to pulsars at high luminosities and consistent with supernova rates.
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Constraining the Pulsar Beaming Fraction with TeV-Selected Galactic Pulsar Wind Nebulae and unidentified TeV Sources
TeV-selected PWNe and unidentified sources yield beaming fractions of 0.1-0.3 across radio, gamma-ray, and X-ray bands, with survey-to-survey differences explained by selection biases or older pulsars and reproducible via time-dependent opening angles.
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How many VHE gamma-ray binaries with young pulsars can be observed?
Population synthesis of pulsar-massive star binaries yields an estimate for the number of observable VHE gamma-ray sources in the Galaxy, incorporating anisotropic wind-interaction zones.
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Evolution of Crab Pulsar: Magnetic Inclination Angle and Spin
The routine model with bulk viscosity best reproduces the Crab pulsar's magnetic inclination angle, spin period, and derivative, while electromagnetic torque and accretion suppress inclination growth and most other effects are negligible.