X-ray observations of GX 17 plus 2 from Uhuru
GX 17 X ray observation, noting exponential spectrum characteristic of thermal bremsstrahlung and resemblance with Sco X-1 radiation
Engineering topics
Publications and source records attributed to Giacconi, R..
GX 17 X ray observation, noting exponential spectrum characteristic of thermal bremsstrahlung and resemblance with Sco X-1 radiation
Coma cluster X ray source data from Uhuru satellite, observing size, luminosity, spectra, thermal bremsstrahlung mass and stability
Large amplitude periodic X ray pulsations from Centaurus X-3, observing abrupt source intensity and pulse rate changes
X ray pulsations from Cygnus X-1 observed from Uhuru satellite, suggesting exstar discovery
X-ray emission from the Cygnus Loop was observed in the energy region around 0.2 to 1 keV with a collector that focused X-rays along one dimension while scanning across the nebula. The total integrated intensity is 13 nanoerg per square centimeter per second. The one-dimensional X-ray structure has the same angular size - about 3 degrees - as the outermost boundaries of the optical filaments. There is no increase in X-ray emission at the center of the nebula nor at the strong feature that is seen in certain radio maps. The X-ray spectrum is consistent with thermal radiation from a hot plasma at a temperature of about 4 million K.
Galactic plane X ray scan by NASA small astronomy satellite Uhuru, discussing satellite instrumentation, detector and sensor sensitivity and preliminary measurements
Cygnus X-1 and X-2 X ray source location from Uhuru satellite measurements
Seyfert galaxies NGC 1275 and NGC 4151 X ray flux detection, determining position and emission intensity
M87, Cen A NGC 5128 and 3C 273 X ray emission observations in Virgo cluster, using Uhuru satellite
Sounding rocket X ray survey of Cassiopeia region for supernova remnants and galactic source distribution
OSO-4 X ray telescope and rotating wheel experiments
Galactic X ray source spectral data observed by rocket, presenting graph with corrections
Grazing incidence telescopes for X ray astronomy, describing mirrors, detection systems and dispersion techniques
Solar flares spectra X ray portion, considering spatial distribution, relation to magnetic fields and time sequence of emitting region
Solar X ray structures during june 8, 1968 flare, using data from rocket-borne grazing incidence telescope
Refurbishment and reflight of instrumented payload on Aerobee rocket for X ray astronomy program
Solar X ray images obtained at solar minimum by grazing-incidence optics, noting X ray radiation spatial distribution is consistent with coronal emission models
Galactic X ray sources from Scorpio to Cygnus, establishing positions of 13 discrete sources