Are Mildly Active Galaxies Sources of e+/- ANNIHILATION Radiation?
Abstract
Mildly active galaxies are examined as possible sources of 511-keV line radiation resulting from electron-positron annihilations. Observations of seven galaxies of various types are made using an HEAO-3 gamma-ray spectrometer. It is shown that none of the galaxies are detected in the 511 keV line and therefore the proposed scaling law for 511-keV line emission from the galactic nuclei is not valid. The results indicate that the scaling overestimates the 511-keV line flux by a factor of 3 or more. Possible causes of this discrepancy are considered. The expected values of and the observed 2.3-sigma upper limits to the 511-keV line flux for each source and the Galactic Center are presented in a table.
- Publication:
-
Positron-Electron Pairs in Astrophysics
- Pub Date:
- July 1983
- DOI:
- Bibcode:
- 1983AIPC..101..303M
- Keywords:
-
- Active Galaxies;
- Galactic Nuclei;
- Galactic Radiation;
- Gamma Ray Astronomy;
- Positron Annihilation;
- Radiation Sources;
- Gamma Ray Spectrometers;
- Heao 3;
- Spaceborne Astronomy;
- Astrophysics;
- 98.70.Qy;
- X-ray sources;
- X-ray bursts