RHESSI results on γ-ray lines from diffuse radioactivity

Details RHESSI results on γ-ray lines from diffuse radioactivity RHESSI results on γ-ray lines from diffuse radioactivity

Feb 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004newar..48...87s&link_type=abstract

New Astronomy Reviews, Volume 48, Issue 1-4, p. 87-91.

Astronomy and Astrophysics

Astrophysics

17

Nuclear Astrophysics, X-Ray And Γ-Ray Spectroscopy

Scientific paper

Although designed to study solar flares, the Reuven Ramaty High Energy Solar Spectroscopic Imager (RHESSI), a NASA satellite, has proven to be sensitive to γ-ray lines generated by recently created radionuclei in the inner Galaxy. I present the current state of this investigation, including flux and line shape measurements of the 1809 keV line from 26Al and a preliminary detection of the lines of 60Fe.

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