Galactic e+-e- annihilation line radiation

Details Galactic e+-e- annihilation line radiation Galactic e+-e- annihilation line radiation

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410..208s&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 208-217 (1997).

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Galactic Center, Bar, Circumnuclear Matter, And Bulge, Gamma-Ray Sources, Gamma-Ray Bursts, Gamma-Ray

Scientific paper

The longest-known and brightest Galactic gamma-ray line is the line at 511 keV from positron annihilation. Despite over two decades of observations, however, the distribution and sources of this line are not well understood. It is only with a steadily increasing database, primarily from OSSE but including other instruments, combined with increasingly sophisticated algorithms to deconvolve image information, that we are now beginning to grasp the shape of the distribution.

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