Centaurus A /NGC 5128/ at 2 keV-2.3 MeV - HEAO 1 observations and implications

Astronomy and Astrophysics – Astronomy

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Cosmic X Rays, Energy Spectra, Galactic Nuclei, Heao 1, Radio Galaxies, X Ray Sources, Active Galaxies, Astronomical Models, Black Holes (Astronomy), Compton Effect, Gamma Ray Astronomy, X Ray Spectra

Scientific paper

The active-nucleus galaxy Centaurus A has been studied at 2 keV-2.3 MeV using data from the UCSD/MIT hard X-ray and low-energy gamma-ray instrument and the GSFC/CIT cosmic X-ray experiment on HEAO-1. It is found that an E exp -1.60 + or - 0.03 power law spectrum breaking to E exp -2.0 + or - 0.2 at 140 keV best describes the January and July 1978 data. The average intensity was 50% higher during the January observations. Upper limits to unresolved lines at 511 keV and 1.6 MeV were found to be 6.5 x 10 to the -4th photons/sq cm-s and 2.2 x 10 to the -4th photons/sq cm-s, respectively, at the 90% confidence level. The present data are consistent with the detailed calculations of the synchrotron self-Compton mechanism; they may also agree, marginally, with the predictions of emission from spherical accretion onto black holes.

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