Early solar system radioactivity and AGB stars

被引：10

作者：

Gallino, R

Busso, M

Wasserburg, GJ

Straniero, O

机构：

[1] Univ Turin, Dipartimento Fis Gen, I-10125 Turin, Italy

[2] Monash Univ, Sch Math Sci, Ctr Stellar & Planetary Astrophys, Clayton, Vic 3800, Australia

[3] Univ Perugia, Dipartimento Fis, I-06123 Perugia, Italy

[4] CALTECH, Div Geol & Planetary Sci, Lunat Asylum, Pasadena, CA 91125 USA

[5] Osservatorio Astron Collurania, I-64100 Teramo, Italy

来源：

NEW ASTRONOMY REVIEWS | 2004年 / 48卷 / 1-4期

关键词：

solar system : formation; stars : AGB and PostAGB;

D O I：

10.1016/j.newar.2003.11.019

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

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 Fe-60, as inferred from recent measurements. (C) 2003 Elsevier B.V. All rights reserved.

引用

收藏

页码：133 / 138

页数：6

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