Astronomy and Astrophysics – Astrophysics
Scientific paper
2003-09-17
Astron.Astrophys.407:L55,2003
Astronomy and Astrophysics
Astrophysics
4 pages, 3 figures
Scientific paper
10.1051/0004-6361:20031056
We report the first measurements of the 511 keV line emission from the Galactic Centre (GC) region performed with the spectrometer SPI on the space observatory INTEGRAL (International Gamma-Ray Astrophysics Laboratory). Taking into account the range of spatial distribution models which are consistent with the data, we derive a flux of $9.9^{+4.7}_{-2.1} \times 10^{-4}$ ph cm$^{-2}$ s$^{-1}$ and an intrinsic line width of $2.95^{+0.45}_{-0.51}$ keV (FWHM). The results are consistent with other high-spectroscopy measurements, though the width is found to be at the upper bound of previously reported values.
Allain M.
Caraveo Patrizia
Cordier Bertand
Diehl Roland
Durouchoux Ph.
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