Models and Observations of the Millimeter and Submillimeter Molecular Line Emission of Bright-Rimmed Clouds
Lecture Planet Formation Topic: Overview of the standard model of planet formation Lecture by: C.P. Dullemond.
The formation of stars and planets Day 2, Topic 1: Giant Molecular Clouds and Gravitational Stability Lecture by: C.P. Dullemond.
IRAC/MIPS view of the ISM: PAHs dominate in IRAC Li & Draine (2001) dust emissivity model; only very strong (> 10 3 x avg.) radiation fields contribute.
Star and Planet Formation
Sternentstehung - Star Formation
Formation of an IMF-Cluster in a Filamentary Layer Collaborators: F. Adams (Michigan), L. Allen (CfA), R. Gutermuth (CfA), J. Jørgensen (CfA), S. T. Megeath.
