TGRS measurements of the positron annihilation spectrum from the galactic center

Computer Science – Performance

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Galactic Center, Bar, Circumnuclear Matter, And Bulge, X- And Gamma-Ray Telescopes And Instrumentation, Gamma-Ray

Scientific paper

The TGRS experiment on board the Wind spacecraft includes a Ge detector with very high resolution (3-4 keV FWHM) at energies around 511 keV. To take advantage of WIND's fixed pointing at the south ecliptic pole and its 3 s rotation, TGRS also includes a Pb occulter fixed on the spacecraft body subtending an arc of 90° along the ecliptic plane. Spectra of the Galactic center region, identified by this occultation method, have been accumulated since 1994 November. In this paper we present updated results for the Galactic center positron annihilation line from these occulted spectra. From the results prior to fall 1997 we obtained the intensity, width, energy and variability of the line, the positronium (Ps) fraction, and limited information about the spatial distribution of the line, all of which have been published. Since the fall of 1997, degradation of the instrument performance has limited us to improving our results for the spatial distribution. These updated results are in marginal disagreement (~2.5σ) with a model based on earlier OSSE measurements. .

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