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Spectral And Intensity Variations Of Galactic Al-26 Emission
ASTRONOMY & ASTROPHYSICS, no. 3 (2009): 713-724
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Abstract
Aims. Gamma-ray line emission from the radioactive decay of Al-26 reflects nucleosynthesis in massive stars and supernovae. We use INTEGRAL Al-26 measurements to characterize the distribution and characteristics of Al-26 source regions throughout the Galaxy.Methods. The spectrometer SPI aboard INTEGRAL has accumulated over five years of d...More
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