Gallino, R. and Busso, M. and Wasserburg, G. J. and Straniero, O. (2004) Early solar system radioactivity and AGB stars. New Astronomy Reviews, 48 (1-4). pp. 133-138. ISSN 1387-6473. doi:10.1016/j.newar.2003.11.019. https://resolver.caltech.edu/CaltechAUTHORS:20131115-152304136
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Abstract
The possible stellar origin of those short-lived nuclei that were shown to be alive in the Early Solar System (ESS) is briefly discussed. The applicability of a close-by AGB star polluting the protosolar nebula depends on the extent to which several nuclei can be explained and in particular the strongly debated problems of the initial amount of ^(60)Fe, as inferred from recent measurements.
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| Additional Information: | © 2003 Elsevier B.V. Included in a Special Issue on Astronomy with Radioactivities IV and Filling the Sensitivity Gap in MeV Astronomy. We thank the Editor, Roland Diehl, for his patience and persistence, Guenther Lugmair, Andrew M. Davis and an anonymous referee for very useful suggestions. Work partly supported by the Italian MURST-FIRB project "The origin of heavy elements beyond Fe". | |||||||||
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| Subject Keywords: | solar system : formation; stars : AGB and PostAGB | |||||||||
| Issue or Number: | 1-4 | |||||||||
| Classification Code: | PACS: 97.60.-s; 96.10.+i | |||||||||
| DOI: | 10.1016/j.newar.2003.11.019 | |||||||||
| Record Number: | CaltechAUTHORS:20131115-152304136 | |||||||||
| Persistent URL: | https://resolver.caltech.edu/CaltechAUTHORS:20131115-152304136 | |||||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | |||||||||
| ID Code: | 42508 | |||||||||
| Collection: | CaltechAUTHORS | |||||||||
| Deposited By: | Tony Diaz | |||||||||
| Deposited On: | 15 Nov 2013 23:42 | |||||||||
| Last Modified: | 10 Nov 2021 16:24 |
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