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From the following article:

An asymmetric distribution of positrons in the Galactic disk revealed by gamma-rays

Georg Weidenspointner, Gerry Skinner, Pierre Jean, Jürgen Knödlseder, Peter von Ballmoos, Giovanni Bignami, Roland Diehl, Andrew W. Strong, Bertrand Cordier, Stéphane Schanne & Christoph Winkler

Nature 451, 159-162(10 January 2008)

doi:10.1038/nature06490

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Figure 1 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 1

A sky map in the 511-keV electron–positron annihilation line, and the sky distribution of hard LMXBs.

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Figure 2 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 2

The longitude profile of a model for the sky distribution of 511-keV electron–positron annihilation line radiation for Galactic latitudes |b| < 10°.

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Figure 3 - Unfortunately we are unable to provide accessible alternative text for this. If you require assistance to access this image, or to obtain a text description, please contact npg@nature.com

Figure 3

Energy spectra of the bold gamma-ray emission from the inner Galactic disk.

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