Derivation of gamma-ray emissivity in the Galaxy from satellite data

Details Derivation of gamma-ray emissivity in the Galaxy from satellite data Derivation of gamma-ray emissivity in the Galaxy from satellite data

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jpha....8..617s&link_type=abstract

Journal of Physics, Part A - Mathematical and General, vol. 8, Apr. 1975, p. 617-623. Research supported by the Science Researc

Astronomy and Astrophysics

Astronomy

25

Emissivity, Galactic Radiation, Gamma Rays, Satellite Observation, Spaceborne Astronomy, Error Analysis, Galactic Nuclei, Milky Way Galaxy, Oso-3, Radiant Flux Density, Sas-2, Statistical Analysis

Scientific paper

A method of deriving the gamma-ray emissivity in the Galaxy by unfolding the longitudinal distribution of gamma-ray intensity is proposed and applied to the available data from the SAS-II and OSO-III instruments. The uncertainties in the analysis resulting from statistical errors in the data are estimated. A broad enhancement of emission 3-8 kpc from the galactic center is found. There is evidence for a drop in emissivity within 3 kpc of the center, although the uncertainties in this region are very large.

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