Synchrotron emission at strong radiative damping
Synchrotron emission of relativistic particle in magnetic field with radiative reaction force comparable to Lorentz force, emphasizing pulsar cosmic ray electron acceleration
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Synchrotron emission of relativistic particle in magnetic field with radiative reaction force comparable to Lorentz force, emphasizing pulsar cosmic ray electron acceleration
Pulsar CP 1919 X ray emission upper limits from balloon flight data, comparing to NP 0532 over entire electromagnetic spectrum
Electronic pulsarium displaying flashing or beeping properties of pulsars
Crab Nebula pulsar NP 0532, describing quasi- sinusoidal oscillation in arrival times of radio pulses
Neutron star superfluid turbulent state, applying dynamic model to conditions in pulsars
X ray sources identification with optical counterparts, noting lack of radio and pulsar type emissions
Sco XR-1 optical intensity power spectra oscillations searched for in pulsar frequencies and fundamental radial mode vibrations in white dwarfs and neutron stars
Synchrotron source spectra natural frequency cut- off in absence of self absorption and electron energy cut-offs, discussing pulsar NP 0532
DSIF operations for testing theory of general relativity by very long baseline interferometers and for study of pulsar polarization
Background radiation in space and synchrotron X radiation in galaxy and pulsars
DSN research and technology support, including radiometric observations, pulsar observations, precision antenna gain measurement, and clock synchronization transmissions
Autocorrelation and power spectrum analysis computer programs for signal analysis of X ray and gamma ray emitting pulsars
Quasi-stellar radio sources similarity to pulsars based on similar characteristics
Crab Nebula and pulsar NP 0532 X ray spectra discussing pulse profile, emission and interstellar absorption
Pulsating gamma ray flux from pulsar NP 0532 in energy range from 250 keV to 2.3 MeV
Pulsar polarization characteristics and pulse profile observations in 250-450 MHz range
Short time variability of intensity of optical pulses from pulsar NP 0532, using telescopes
Neutron star models, discussing crystalline crust, particle superfluid properties, rotational vortices and relation to Crab Nebula pulsar