X-ray and optical observations of the pulsar NP 0532 in the Crab Nebula.
Pulsar NP 0532 in Crab Nebula observed by rocket and telescope showing strong pulsed X ray signal
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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
Crab Nebula pulsar light intensity fluctuations on very short time scale, noting negative observations
Pulsars pulse duration and shape as key to neutron stars linkage with supernova explosions
Unified model for pulsars involving electron population inversion and laser type transition
Pulsars pulse arrival time measured using cesium clock during weekly observations