Busemann, H.; Bühler, F.; Agafonov, Y. N.; Baur, H.; Bochsler, P.; Eismont, N. A.; Heber, V. S.; Wieler, R. and Zastenker, G. N.
PDF (Not Set)
- Requires a PDF viewer such as GSview, Xpdf or Adobe Acrobat Reader
|Google Scholar:||Look up in Google Scholar|
Introduction: The composition of the present interstellar medium (ISM) provides an important benchmark in cosmochemistry. It serves as a reference for galactic chemical evolution (GCE) models, solar mixing predictions and provides information for understanding Big Bang nucleosynthesis. The present-day ISM 3He abundance allows, combined with the protosolar 3He, deduced from the Jovian atmosphere or meteorites [1,2], tracing the GCE over the past 4.56 Ga. 3He/4He = (2.5 0.6) x 10-4 has been determined for the local ISM . However, the uncertainty is too large to better constrain GCE models and - in combination with the present-day solar wind value - the protosolar D/H .
|Item Type:||Conference Item|
|Extra Information:||Abstract #5170|
|Academic Unit/Department:||Science > Physical Sciences
|Depositing User:||Kyra Proctor|
|Date Deposited:||02 Jul 2007|
|Last Modified:||16 Jan 2016 10:00|
|Share this page:|