Ariel 5 hard X-ray measurements of galactic and extragalactic X-ray sources

Astronomy and Astrophysics – Astronomy

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Ariel 5 Satellite, Crab Nebula, Galactic Radiation, Novae, Satellite-Borne Instruments, X Ray Sources, Astronomical Models, Black Holes (Astronomy), Light Curve, Power Spectra, Pulsars, Scintillation Counters, X Ray Astronomy, X Ray Spectra

Scientific paper

The paper reviews the program of measurement and interpretation associated with the output of the hard X-ray sensor aboard Ariel 5, with emphasis on distinguishing various forms of power-law and thermal spectra. The sensor, a CsI crystal scintillator detector covering the range from 26 keV to 1.2 MeV, is described in detail. Observations are reported for the Coma cluster source, several galactic-center sources, the Crab Nebula, Her X-1, and the transient sources A1118-61 and A0535+26. Hard X-ray observations are discussed along with possible production mechanisms for the black-hole candidates A0620-00 and Cyg X-1. The Cyg X-1 transition of May 9, 1975, is examined in terms of an inverse-Compton acceleration model that is analogous to the Fermi acceleration mechanism for cosmic rays.

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