On the pulsation hypothesis for massive red supergiants
Red supergiant pulsar hypothesis using Q values derived from stellar luminosity, period, and spectrum
Stothers, R.↗
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Search indexed NASA NTRS and DOE OSTI research on propulsion, heat transfer, battery materials and energy systems. Follow report and document links to the original sources.
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Simultaneous observations of a pulsating radio source over a 5,000 km baseline.
Pulsar CP 1919 observed simultaneously at Arecibo and Stanford, discussing interstellar scintillation as possible explanation for amplitude variations
Comella, J. M.↗
Telecommunications Division
Spacecraft telecommunication systems - coding methods for phase locked loops, absolute time determination by pulsar, communications elements research
Source record↗
Simultaneous optical and radio observations of NP 0532
Simultaneous optical and radio observations of Crab Nebula pulsar NP 0532 and time delay analysis
Conklin, E. K.↗
Pulsed X-ray emission of NP 0532 in March 1968
Pulsed X ray emission of pulsar NP 0532 in Crab Nebula
Boldt, E. A.↗
The instability of stellar structures intermediate between white dwarfs and neutron stars.
Instability of stellar structures intermediate between white dwarfs and neutron stars shown by stellar models, discussing pulsar signals periodicities
Cameron, A. G. W.↗
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.↗
Simultaneous optical and radio observations of NP 0532.
Crab Nebula pulsar NP 0532 simultaneous optical and radio observations, noting influence of interstellar dispersion value uncertainty
Conklin, E. K.↗
Hydromagnetic plasma acceleration by rapidly rotating astrophysical objects.
Plasma acceleration away from rotating magnetized astrophysical objects analyzed and applied to pulsar NP 0532 for magnetic moment and mass loss rate calculations
Michel, F. C.↗
Mass loss from pulsating neutron stars.
Radial pulsations of neutron star losing mass, interpreting Crab Nebula pulsar observed period and secular increase of period
Stothers, R.↗
Pulsed X-ray emission of NP 0532 in March 1968.
Pulsed X ray emission associated with pulsar NP 0532 in Crab Nebula measured by six element detector on Aerobee 150 rocket
Boldt, E. A.↗
Interstellar polarization of starlight and the turbulent structure of the Galaxy.
Polarization fluctuations of starlight indicating turbulent structure of interstellar medium, noting pulsar signal dispersion and Faraday rotation
Jokipii, J. R.↗
Alignment of oblique rotators
Pulsars with torque aligning magnetic moment with spin axis
Goldwire, H. C., Jr.↗
The effects of nuclear forces on the maximum mass limit of neutron stars
Maximum mass limit effects of stable neutron stars on pulsar models
Tsuruta, S.↗
Electric fields in rotating, magnetic, relativistic stars
Electric fields in rotating magnetic relativistic neutron stars, analyzing static fields in corotating frame and pulsar emission
Demianski, M.↗
Relativistic stellar-wind torques
Solar wind-induced torque calculated considering special and general relativistic effects, extending method to pulsar rotational model
Michel, F. C.↗
Disintegration and energy degradation of very high-energy cosmic rays in intense photon fields
Very high energy cosmic rays disintegration and energy degradation by intense blue shifted photon fields of supernovae quasars and pulsar models
Pollack, J. B.↗
Alignment of oblique rotators
Pulsar slowdown by radiation field torques indicated by alignment torque in magnetized oblique sphere rotating in vacuum
Goldwire, H. C., Jr.↗