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Titlebook: Non-Solar X- and Gamma-Ray Astronomy; L. Gratton Book 1970 International Astronomical Union 1970 astronomy.instruments.neutron star.observ

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The Flux of Hard Radiation from M87,f hard radiation from the general direction of Virgo; the experiment discussed here, conducted 16 months later, recorded approximately the same flux from a smaller region of sky that tends to isolate M87 as the most likely candidate for the source.
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A Rocket Observation of Cosmic X-rays in the Energy Range between 0.15 and 20 keV,g rocket scanned a celestial region in which the galactic latitude .. changed from 30° to −55° across the galactic plane in the Cygnus-Cassiopeia region. The spectrum of Cyg XR-2 thus obtained is represented by a thermal bremsstrahlung of temperature 3.4 keV modified by the interstellar absorption f
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978-94-010-3313-8International Astronomical Union 1970
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Non-Solar X- and Gamma-Ray Astronomy978-94-010-3311-4Series ISSN 1743-9213 Series E-ISSN 2352-2186
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Techniques for Improving the Sensitivity of Proportional Counters Used in X-ray Astronomy,n the energy range from 1 to 50 keV, proportional counters have advantages over other types of detectors; they provide energy resolution and they can be made relatively easily with very large window areas.
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