Short-lived nuclei in the Galaxy and in the early solar system: crucial tests expected from gamma-ray line observations

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dc.creatorBusso, Maurizio
dc.creatorCiprini, Stefano
dc.creatorMarcucci, Francesca
dc.date2003-08-21
dc.date2003-08-22
dc.date.accessioned2026-07-07T02:09:17Z
dc.date.available2026-07-07T02:09:17Z
dc.descriptionWe discuss some open problems in the understanding of the Early Solar System abundances of short-lived radioactive isotopes, and the important clarification expected on this matter by precise measurements of the average galactic abundances of 26Al and 60Fe, through their gamma-ray lines.
dc.description7 pages, 1 tab. 1 fig. In ''Science with the New Generation of High Energy Gamma-ray Experiments'' Edited by S. Ciprini, A. De Angelis, P. Lubrano and O. Mansutti. August 2003, Udine: Forum Publ., p. 63 (Proc. of a Workshop held in Perugia, Italy, May 21-22, 2003)
dc.identifierhttps://arxiv.org/abs/astro-ph/0308374
dc.identifierhttp://arxiv.org/abs/astro-ph/0308374
dc.identifierScience with the New Generation of High Energy Gamma-ray Experiments, Forum special publ., August 2003, p. 63
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/6376
dc.subjectAstrophysics
dc.titleShort-lived nuclei in the Galaxy and in the early solar system: crucial tests expected from gamma-ray line observations
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