Some recent results of X-ray astronomy
X ray astronomy rocket experiment for identification and positioning of SCO X-1 strong X ray source
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X ray astronomy rocket experiment for identification and positioning of SCO X-1 strong X ray source
Relativistic electron energy loss due to inverse Compton scattering from cosmological blackbody radiation, noting diffuse X ray background implication for electron source strength
X ray astronomy data from rocket- and balloon- borne instruments including sources detection, identification and variability
X ray source Sco X-1, discussing stellar evolution and possible time variations in X ray flux
Hard solar and cosmic X rays observed by OSO 3, noting Lupus XR-1 and galaxy M 87 sources
Modulation collimators determining angular sizes and celestial positions of X ray sources Sco X-1 and Taurus XR-1
X ray emission from Seyfert galaxy nuclei, noting model with bremsstrahlung from hot source
Low energy X ray spectra of Sco X-1 and Sagittarius sources measured by Be and Al window proportional counters during rocket flight
Weak X ray sources at 20-100 Kev photon energies observed during balloon flight, finding hard rays from Ara XR-1 and Nor XR-1
High energy X ray observational data for Sagittarius sources scanned by active telescope during February 1968 balloon flight
Galactic X ray source spectral data observed by rocket, presenting graph with corrections
Interstellar absorption of 10 A X rays from sources in Scorpio-Sagittarius region, noting gas density between earth and Crab Nebula
X ray source from Coma cluster of galaxies, interpreting observed flux on basis of missing mass suggested by Virial theorem
Cosmic rays and cosmic X rays, considering galactic and extragalactic sources, diffuse background, detection devices, etc
X and gamma ray astronomy instrumentation, point sources, continuum emission, line spectra, etc
Hard X ray experiment for Astronomical Netherlands Satellite to detect and measure X ray sources and line emission
Statistical analysis of X ray line emission from cosmic radiation source
X ray background angular structure comparison with optical galaxies spatial distribution, ruling out universe models with sources following cosmological mass distribution