Acceleration of high-energy cosmic rays by pulsars.
High energy cosmic ray origin and acceleration by LF electromagnetic radiation produced by pulsars, noting maximum energy for protons
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High energy cosmic ray origin and acceleration by LF electromagnetic radiation produced by pulsars, noting maximum energy for protons
Crab Nebula pulsar detection by TV camera with image intensifier at focus of astronomical telescope, detailing instrumentation and observations
Pulsars and ancient chinese records of supernova explosions, relating luminous intensities, radio sources and evolution
Pulsar PSR 0833-45 period decrease and rate of change in period increased between 24 February-3 March 1969, discussing contraction explanation
Pulsar NP 0532 in Crab Nebula observed by rocket and telescope showing strong pulsed X ray signal
IR and optical measurement of Crab pulsar NP 0532, analyzing energy density per pulse and smoothness of visual data
Pulsars observed for average energies at centimeter wavelengths, using azimuth elevation antenna
Night sky Cerenkov light detectors observations of pulsars CP 1133, NP 0532 and NP 0527, noting instrumental limitation in detecting ultrashort light pulses
Optical observations of pulsar NP 0532, comparing light curves in IR and UV, noting polarization
Quasar features compared to pulsars, noting complete analogy except for energy output scale
Optical detection of pulsars with emphasis on CP 1919, discussing optical variation
Crab Nebula pulsars radio properties, possible neutron star origin, interstellar gas and magnetic fields, etc
Mean and variance of Faraday rotation and pulsar signal dispersion in galactic turbulent structure, applying to statistically homogeneous disk model of Galaxy
Pulsar model with seat as rotating neutron star having dipolar magnetic field not parallel to rotation axis
Rotating neutron stars, pulsars and cosmic X ray sources, accounting for large and small diameter sources by rotating neutron star losing mass in magnetic field
Pulsars and X ray emitting supernova remnants
Pulsed high energy X rays from Crab Nebula pulsar NP 0532 measured by balloon-borne X ray telescope
Random variations of terrestrial rotation rate effects on pulsar observations, discussing methods to minimize effects