SMM detection of interstellar Al-26 gamma radiation

Details SMM detection of interstellar Al-26 gamma radiation SMM detection of interstellar Al-26 gamma radiation

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..353s&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 353-356 (SEE N85-33902 22-93)

Physics

Aluminum Isotopes, Cosmic Rays, Flux Density, Gamma Rays, Interstellar Matter, Spatial Distribution, Galactic Radiation, Half Life, Heao 3, Magnetic Rigidity, Solar Flares, Solar Maximum Mission, Time, Zenith

Scientific paper

The gamma-ray spectrometer on the Solar Maximum Mission Satellite has detected the interstellar 26Al line when the Galactic center traversed its aperture in 1980, 1981, 1982, and 1984. The center of the emission is consistent with the location of the Galactic center, but the spatial distribution is presently not well defined. The total flux in the direction of the Galactic center is (4.3±0.4)×10-4γ/cm2 s rad for an assumed population I distribution.

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