Gamma-Ray Line Emission from 7-Li and 7-Be Production by Cosmic-Rays

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dc.creatorTatischeff, V.
dc.creatorThibaud, J. -P.
dc.creatorKiener, J.
dc.creatorCasse, M.
dc.creatorVangioni-Flam, E.
dc.date2001-04-03
dc.date.accessioned2026-07-07T01:58:08Z
dc.date.available2026-07-07T01:58:08Z
dc.descriptionWe calculate the total gamma-ray line emission at ~450 keV that accompanies 7-Li and 7-Be production by cosmic-ray interactions, including the delayed line emission at 0.478 MeV from 7-Be radioactive decay. We present a new gamma-ray spectroscopic test which has the potential to give direct information on the nature of the interstellar regions into which 7-Be ions propagate and decay. Finally, we evaluate the intensity of the predicted diffuse emission from the central radian of the Galaxy.
dc.description4 pages with 5 figures. Contributed paper at the 4th INTEGRAL Workshop, 4-8 September 2000, Alicante (Spain). To be published in the ESA-SP series. Uses esapub.cls
dc.identifierhttps://arxiv.org/abs/astro-ph/0104051
dc.identifierhttp://arxiv.org/abs/astro-ph/0104051
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2654
dc.subjectAstrophysics
dc.titleGamma-Ray Line Emission from 7-Li and 7-Be Production by Cosmic-Rays
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