| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1780495 | New Astronomy Reviews | 2006 | 4 Pages |
Abstract
Establishing the origin of short-lived radionuclides (SRs) with half-lives ∼Ma has important consequences for the astrophysical context of our sun’s birth place. I discuss here the different explanations that can account for the roster of SRs present in the solar accretion disk 4.57 Ga ago, emphasizing on their dependence on the poorly known initial value of SRs.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Matthieu Gounelle,