Condensation of Forsterite and Metallic Iron Around Evolved and Young Stars

Details Condensation of Forsterite and Metallic Iron Around Evolved and Young Stars Condensation of Forsterite and Metallic Iron Around Evolved and Young Stars

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.

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