Projection on the galaxy anticenter in the light of MeV-gamma radiation and the search for gamma emission from radiopulsars

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Galactic Radiation, Gamma Rays, Pulsars, Bremsstrahlung, Compton Effect, Crab Nebula, Disk Galaxies, Gamma Ray Bursts, High Altitude Balloons, Radio Bursts

Scientific paper

Two compton telescope carrying balloon flights for the measurement of cosmic MeV-gamma radiation and gamma emission from radiopulsars, are reported on. A clearly enhanced gamma emission is observed in the galactic length domain between 160 and 197 deg arc and is partially due to the Crab nebula plus pulsar. Electron Bremsstrahlung is mainly responsible for MeV-gamma quanta from the anticentrum direction. The electron spectrum bends at about 30 MeV. The low energy gamma domain is determined with a significance of 6.5 sigma. Pulses in the gamma and the Rontgen domain are in phase. The measured light curve of the 0950 + 08 pulsar shows two maxima and has the same profile as the gamma pulsars Crab and Vela.

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