Physics
Scientific paper
Mar 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006lpi....37.1636n&link_type=abstract
37th Annual Lunar and Planetary Science Conference, March 13-17, 2006, League City, Texas, abstract no.1636
Physics
Scientific paper
Growth of metallic iron and forsterite grains around evolved and young
stars are studied by using experimentally obtained condensation
coefficients, which results in smaller grain size of forsterite than
metallic iron due to smaller coefficients.
Ikeda Yasufumi
Nagahara Hiroki
Ozawa Kazuhito
Tachibana Shogo
No associations
LandOfFree
Condensation of Forsterite and Metallic Iron Around Evolved and Young Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with Condensation of Forsterite and Metallic Iron Around Evolved and Young Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Condensation of Forsterite and Metallic Iron Around Evolved and Young Stars will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1143591