Model calculations for the production of the short-lived nuclides 10 Be, 26 Al, 41 Ca and 53 Mn by solar energetic particles (SEP) in the asteroidal region during the early evolution of the solar system are presented. Based on the results of these calculations and the initial solar system abundances
β¦ LIBER β¦
Short-lived nuclides in the early solar system: the stellar connection
β Scribed by J.N. Goswami
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 221 KB
- Volume
- 48
- Category
- Article
- ISSN
- 1387-6473
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
Low energy particle production of short-
β
K.K. Marhas; J.N. Goswami
π
Article
π
2004
π
Elsevier Science
π
English
β 203 KB
Multiple sources or late injection of sh
β
N. Dauphas
π
Article
π
2005
π
Elsevier Science
π
English
β 135 KB
Short-lived nuclei in the early Solar Sy
β
G.J. Wasserburg; M. Busso; R. Gallino; K.M. Nollett
π
Article
π
2006
π
Elsevier Science
π
English
β 987 KB
On non-thermal nucleosynthesis of Short-
β
Jean Duprat; Vincent Tatischeff
π
Article
π
2008
π
Elsevier Science
π
English
β 267 KB
The first results from the STARDUST mission revealed that refractory phases formed at a close distance from the nascent Sun have been transported to the comet forming region. Such refractory phases from meteorites (that originate from the asteroid belt), hold the ashes of Short-Lived Radionuclei (SL
The origin of short-lived radionuclides
β
Matthieu Gounelle
π
Article
π
2006
π
Elsevier Science
π
English
β 127 KB
An adaptation of the pulser method for t
β
W. GΓΆrner
π
Article
π
1974
π
Elsevier Science
β 84 KB