First significant detection of gamma-ray pulsed radiation variations associated with a glitch in PSR J0205+6449, with changes in peak amplitude ratio and separation attributed to magnetospheric reconfiguration.
I - Outer magnetosphere gaps
6 Pith papers cite this work, alongside 827 external citations. Polarity classification is still indexing.
6
Pith papers citing it
827
external citations · OpenAlex
citation-role summary
dataset 1
citation-polarity summary
fields
astro-ph.HE 6years
2026 6roles
dataset 1polarities
use dataset 1representative citing papers
The Guitar nebula's pulsar appears to accelerate electrons to within ~3/4 of the theoretical maximum potential, and its brightness is best explained by the pulsar crossing an old supernova remnant's compressed, magnetized shell.
Magnetic inclination alignment with timescale proportional to B to the minus two suppresses observed numbers of strong-field neutron stars, unifying pulsars and magnetars under one log-uniform initial B distribution.
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.
Observational evidence links obscured super-Eddington accretion to slower precessing jets in stellar-mass compact object systems, contrasting with fixed fast jets in low-density environments.
Uses synchro-curvature framework and observed cutoff energies to determine equilibrium Lorentz factors and pitch angles, offering a physical account of the L_gamma proportional to E_dot^0.68 trend.
citing papers explorer
-
Discovery of Short-Term {\gamma}-Ray Pulsed Radiation Variations Following a Glitch in PSR J0205+6449
First significant detection of gamma-ray pulsed radiation variations associated with a glitch in PSR J0205+6449, with changes in peak amplitude ratio and separation attributed to magnetospheric reconfiguration.
-
Guitar Nebula: extreme accelerator in extreme environment
The Guitar nebula's pulsar appears to accelerate electrons to within ~3/4 of the theoretical maximum potential, and its brightness is best explained by the pulsar crossing an old supernova remnant's compressed, magnetized shell.
-
A Log-Uniform Initial Magnetic Field Distribution Explains Pulsar and Magnetar Populations through Magnetic Inclination Alignment
Magnetic inclination alignment with timescale proportional to B to the minus two suppresses observed numbers of strong-field neutron stars, unifying pulsars and magnetars under one log-uniform initial B distribution.
-
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.
-
The link between obscured accretion and mildly relativistic precessing jets
Observational evidence links obscured super-Eddington accretion to slower precessing jets in stellar-mass compact object systems, contrasting with fixed fast jets in low-density environments.
-
A synchro-curvature treatment of gamma-ray luminosity trends in pulsars
Uses synchro-curvature framework and observed cutoff energies to determine equilibrium Lorentz factors and pitch angles, offering a physical account of the L_gamma proportional to E_dot^0.68 trend.