PPT Slide
Star Formation June 1999, Nagoya
ROSAT All-Sky Survey, wTTS Halos, Goulds Belt, nearby young stars
Star forming region kinematics, jets
Binary fractions and distributions
Cloud collapse calculations:
- multiple fragmentation common, collapse scale from 0.01pc to 100AU
- various geometries and velocity fields investigated, robust
- various geometries and velocity fields investigated, robust
- weakly hierarchical, or non-hierarchical outcomes
- classic problem, but only N=3 well-studied with modern codes
- star formation questions not addressed
Statistical characterization of complete decay by in-depth analysis of remnants