On the powerful X-ray emission of radiogalaxies
Radio galactic emission and cosmic X-radiation
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Radio galactic emission and cosmic X-radiation
Nuclear emulsion, scintillation photodosimeter, and x-ray film for measurement of cosmic radiation dose in vostok iii and iv spacecraft
Angular diameters of X-ray source regions in Scorpio and Sagittarius constellations by rocket measurement with collimator
Of and Wolf-Rayet stars high temperature envelopes as cosmic thermal X ray sources, discussing continuous mass loss from spectrophotometry data
Mechanism for production of X-rays and gamma rays in galaxies noting photon and electron spectrum
Mechanism for production of X-rays and gamma rays in galaxies, noting photon and electron spectrum
Location of X-ray source Sco X-1 determined by instrumented payload flown on stabilized Aerobee rocket
Explosive limb flare of November 20, 1960 shown to coincide with beginning of radio and X-ray emission
X-ray and gamma ray astronomy, discussing observational methods, physical processes of generation, radiation intensity, etc
Neutron stars considered as origin of X-ray emission from Scorpius and Crab Nebula
Interstellar X-ray absorption edges due to K- shell photoionization of oxygen and neon, using element abundances and atomic photoelectric cross section data
Suprathermal X ray bremsstrahlung from proton-electron collisions in galactic and solar cosmic radiation
Solar X ray flare of July 7, 1966 with Explorer 33 satellite atributed to McMath plage region 8362, discussing solar and cosmic radio noise
X ray polarization from Sco X-1, noting spurious instrumental polarization due to cosmic ray anisotropy using X ray polarimeter
Scorpius XR-1 X ray emission spectra, discussing Fe emission line near 7 kev plasma models, supernova mass and cosmic abundance
X ray line emission from Sco X-1 using Monte Carlo estimates of spectral distribution of scattered photons in terms of Fe line and cosmic abundance
X rays from Sco XR-1 compared with galactic cosmic rays and solar Lyman alpha radiation to determine ionospheric ionization causing radio wave attenuation