The X-ray spectra of Cygnus XR-1 and the Crab Nebula.
Crab Nebula and Cygnus XR-1 X ray spectra shown to have differential number power law spectra and same intensity
Peterson, L. E.↗
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Possible conversion of rotational energy of the neutron star in the Crab Nebula into energy of relativistic electrons.
Rotational energy conversion of neutron star into relativistic electrons energy suggested by increasing period of pulsating radio source in Crab Nebula
Finzi, A.↗
Crab Nebula pulsar NP 0532.
Crab Nebula pulsar properties including pulse shape, dispersion and strong pulse emission
Comella, J. M.↗
Condensed objects in the Crab Nebula.
Condensed supernova remnants in Crab Nebula, considering various hypotheses for radio source
Burbidge, G.↗
Television detection of the Crab Nebula pulsar.
Crab Nebula pulsar detection by TV camera with image intensifier at focus of astronomical telescope, detailing instrumentation and observations
Miller, J. S.↗
Photoelectric spectrophotometry of the Crab pulsating radio source NP 0532.
Crab Nebula pulsar NP 0532 photoelectric spectrophotometry results, noting main pulse and interpulse spectral energy distributions similarity to extended synchrotron radiation
Oke, J. B.↗
X-ray pulsar in the Crab Nebula.
X ray pulsations in Crab Nebula at frequency closely matching radio and optical pulsations, noting energy distribution
Chubb, T. A.↗
2-20 kev spectrum of X-rays from the Crab Nebula and the diffuse background near galactic anticenter.
X ray energy spectrum from Crab Nebula and diffuse background on celestial sphere near galactic anticenter, noting spectral index
Boldt, E. A.↗
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
Bradt, H.↗
Infrared and optical measurements of the Crab pulsar NP 0532.
IR and optical measurement of Crab pulsar NP 0532, analyzing energy density per pulse and smoothness of visual data
Becklin, E. E.↗
Acceleration of ultrarelativistic electrons in the Crab Nebula.
Ultrarelativistic electron acceleration in Crab Nebula maintaining synchrotron spectrum, obtaining power from compressional motion damping, gyrorelaxation effect and pitch angle anisotropy removal
Melrose, D. B.↗
The Crab Nebula ancient history and recent discoveries
Crab Nebula as thin plasma cloud containing weak magnetic field with strongly magnetized neutron star
Rossi, B. B.↗
Hard X-rays from the Crab pulsar.
Pulsed high energy X rays from Crab Nebula pulsar NP 0532 measured by balloon-borne X ray telescope
Floyd, F. W.↗
Search for rapid fluctuations in light from the Crab Nebula pulsar
Crab Nebula pulsar light intensity fluctuations on very short time scale, noting negative observations
Hegyi, D.↗
Coherent synchrotron emission in the Crab Nebula
Coherent synchrotron emission in Crab Nebula associated with electron gyromotion, discussing models for high energy particle acceleration
Caroff, L. J.↗
The Crab Nebula
Crab Nebula continuing energetic activity study indicating origin in nebula center and association with supernova remnant
Melrose, D. B.↗
X-ray scattering by grains in the direction of the Crab pulsar and Sco XR-1
X ray scattering by interstellar grains in direction of Crab pulsar and Sco XR-1
Bowyer, C. S.↗
Shape of the Crab pulsar and its period fluctuations
Crab pulsar /neutron star NP 0532/ possible spherical asymmetry indicated by pulse arrival time anomalies
Chiuderi, C.↗