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- W4230050459 abstract "Observations of the time-dependent, electron-positron annihilation line radiation and gamma-ray continuum emission from the region of the Galactic Center show that there are two components to the annihilation line emission: a variable, compact source at or near the Galactic Center, and a steady, diffuse interstellar distribution. We suggest that the annihilating positrons in the compact source, observed from 1977 through 1979, result from photon-photon pair production, most likely around an accreting black hole, and that the annihilating, interstellar positrons result from the decay of radionuclei produced by thermonuclear burning in supernovae." @default.
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- W4230050459 date "1989-01-01" @default.
- W4230050459 modified "2023-09-30" @default.
- W4230050459 title "Annihilation Radiation and Gamma-Ray Continuum from the Galactic Center Region" @default.
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- W4230050459 doi "https://doi.org/10.1017/s0074180900187091" @default.
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