Observation of Centaurus A in the MeV gamma range

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Centaurus Constellation, Galactic Nuclei, Galactic Radiation, Gamma Ray Astronomy, Active Galactic Nuclei, Balloon Sounding, Balloon-Borne Instruments, Charts, Gamma Ray Telescopes, Monte Carlo Method

Scientific paper

The active galactic nucleus of Cen A was observed in the range of low energy (0.7 to 20 MeV) gamma radiation. The measurements were conducted in a balloon campaign using a Compton telescope. The identification of the source used an imaging technique called the pi-method. In order to simplify the source identification in the pi-charts, these are compared with model charts resulting from Monte Carlo calculations. A thorough understanding of the telescope characteristics (especially the point image function) was decisive for the development of the pi-method. The determined spectral index and the magnitude of the excess agree very well with measurement in the hard X-ray range. The measurement, however, surprises by the significant photon flux in the high energy part of the spectrum, confirming that the luminosity of Cen A in the MeV gamma range is larger than in any other part of the electromagnetic spectrum. Three models to explain the measured spectrum are discussed.

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