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: Raw Spectrum of the Galactic 511 keV line from INTEGRAL SPI Data, also shown are the background model components (Jean, et al 2003, A&A 407, L55). The line width constrains models involving explosive injection of positrons in to the ISM.
Raw Spectrum of the Galactic 511 keV line from INTEGRAL SPI Data, also shown are the background model components (Jean, et al 2003, A&A 407, L55). The line width constrains models involving explosive injection of positrons in to the ISM.

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