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Early solar system radioactivity and AGB stars

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. 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.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1016/j.newar.2003.11.019DOIArticle
http://www.sciencedirect.com/science/article/pii/S1387647303002823PublisherArticle
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".
Funders:
Funding AgencyGrant Number
MURST-FIRB (Italy)UNSPECIFIED
Subject Keywords:solar system : formation; stars : AGB and PostAGB
Issue or Number:1-4
Classification Code:PACS: 97.60.-s; 96.10.+i
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:03 Oct 2019 05:59

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