SIMBAD references

2011A&A...531A..56D - Astronomy and Astrophysics, volume 531A, 56-56 (2011/7-1)

Searching for the 511 keV annihilation line from galactic compact objects with the IBIS gamma ray telescope.

DE CESARE G.

Abstract (from CDS):

The first detection of a gamma ray line with an energy of about 500keV from the center of our Galaxy dates back to the early seventies. Thanks to the astrophysical application of high spectral resolution detectors, it was soon clear that this radiation was due to the 511keV photons generated by electron-positron annihilation. Even though the physical process are known, the astrophysical origin of this radiation is still a mystery. The spectrometer SPI aboard the INTEGRAL gamma-ray satellite has been used to produce the first all-sky map in light of the 511keV annihilation, but no direct evidence of any 511keV galactic compact objects has been found. Owing to its moderate angular resolution, these SPI data are still compatible with a distribution of point sources clustered in the bulge of our Galaxy. Thanks to the fine angular resolution and the large field of view, the IBIS imager on the INTEGRAL satellite gives us the unique opportunity to search for a possible 511keV line from point sources associated to known objects, such as X-ray binaries, or supernovae, or even new ones. We present the first deep IBIS 511keV all-sky map, obtained by applying standard analysis to about 5 years of data. Possible 511keV signals are also searched over hour-day-month timescales. The IBIS sensitivity at 511keV depends on the detector quantum efficiency at this energy and on the background. Both these quantities were estimated in this work. We find no evidence of Galactic 511keV point sources. With an exposure of 10Ms, in the center of the Galaxy, we estimate a 1.6x10–4ph/cm2/s flux 2 sigma upper limit. A similar limit is given in a wide area in the Galactic center region with similar exposures. The IBIS 511keV flux upper limits for microquasars and supernova remnants detected in the hard X domain (E>20keV) are also reported. Our results are consistent with a diffuse e+e annihilation scenario. If positrons are generated in compact objects, we expect that a significant fraction of them propagate in the interstellar medium before they are annihilated away from their birth places.

Abstract Copyright:

Journal keyword(s): methods: data analysis - Galaxy: bulge - gamma rays: diffuse background - X-rays: binaries

Simbad objects: 24

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