Positron astronomy with SPI/INTEGRAL

Details Positron astronomy with SPI/INTEGRAL Positron astronomy with SPI/INTEGRAL

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008newar..52..454w&link_type=abstract

New Astronomy Reviews, Volume 52, Issue 7-10, p. 454-456.

Astronomy and Astrophysics

Astronomy

11

95.85.Pw, 78.70.Bj, 98.35.Ln, 98.38.Am

Scientific paper

We provide an overview of positron astronomy results that have been obtained using the INTEGRAL spectrometer SPI, and discuss their implications for the still mysterious origin of positrons in our Galaxy. It has long been known that the 511 keV positron annihilation emission is strongest from the central region of our Galaxy. Recently, it has been discovered with the SPI spectrometer that the weaker 511 keV line emission from the inner Galactic disk appears to be asymmetric, with the emission to the west of the Galactic center being about twice as strong than that to the east. This distribution of positron annihilation resembles that of low mass X-ray binaries as observed with the INTEGRAL imager IBIS at hard X-ray energies, suggesting that these systems could provide a significant portion of the positrons in our Galaxy. In addition, the spectrometer SPI has permitted unprecedented spectroscopy of annihilation radiation from the bulge and disk regions of the Galaxy, which commences to yield important insights into the conditions of the medium in which the positrons annihilate.

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