The galactic gamma-ray flux in the 0.06 to 5 MeV range

Details The galactic gamma-ray flux in the 0.06 to 5 MeV range The galactic gamma-ray flux in the 0.06 to 5 MeV range

Aug 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978grsa.rept..190g&link_type=abstract

In its Gamma Ray Spectry. in Astrophys. p 190-206 (SEE N78-31971 22-88)

Astronomy and Astrophysics

Astronomy

6

Astronomical Spectroscopy, Emission Spectra, Flux Density, Galactic Radiation, Gamma Ray Astronomy, Gamma Rays, Apollo 16 Flight, Energy Levels, Luminosity, X Ray Density Measurement

Scientific paper

Gamma ray emission from the longitude range -50 deg less than or equal to lambda less than or equal to 22 deg recorded by the Apollo gamma-ray spectrometer and by individual observers is discussed. Agreement of the galactic emission spectra near 1 MeV with hard X-ray observations of the galactic central regions suggests that an ensemble of point sources is responsible for the emissions. Apollo 16 upper limits to the cosmic 4.4 MeV line flux imply that the ratio of line strength to continuum emission for the region observed by Haymes et al is higher than the galactic average.

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