Adriana Rossi General equation VASCO code assumptions and solution
Dust Growth in Transitional Disks
Estimate* the Total Mechanical Feedback Energy in Massive Clusters Bill Mathews & Fulai Guo University of California, Santa Cruz *~ ±15-20% version 2.
MODELING INTRACLUSTER MEDIUM AND DARK MATTER IN GALAXY CLUSTERS Elena Rasia Dipartimento di Astronomia Università di Padova Padova, April 9th, 2002.
IFE proposed for BepiColombo/MPO
