Table of ContentsObserving Star-Formation From the Interstellar Medium to Star-Forming Cores On-Line Version, 1999 Observing Star Formation From the ISM to Star-Forming Cores History: Theory and Optical Observations PPT Slide Important Distinction to Keep in Mind Spectral-Line Mapping Adds Velocity Dimension Orion: 13CO Channel Maps Molecular Outflows Jeans Mass, Virial Mass, and Filling Factors in the ISM What do we need to explain? Self-similar Structure on Scales from 100 pc to 0.1 pc...in Orion �Clump� Mass Distribution �Larson�s Law� Scaling Relations (1981) PPT Slide Rough Virial Equilibrium in Star-forming regions Density-Velocity-Magnetic Field Structure Velocity Structure Velocity Coherent Cores* Where does the self-similarity end? PPT Slide Similar �Transition� Found in Spatial Distribution of Stars PPT Slide Magnetic Field Structure Using Polarization to Map Magnetic Fields Using Polarimetry to Map Field Structure PPT Slide Magnetic Field Structure: Emission Polarimetry Cloud Lifetimes The Effects of a Previous Generation of Stars Density-Velocity-Magnetic Field Structure Initial Conditions for Star-Formation (Version 99) PPT Slide Thanks to: What now? The Pleiades Bright Nebula: Orion Dark Nebula: The Horsehead The Electromagnetic Spectrum A Dense Core: L1489 A Dark Cloud: IC 5146 |
Author: Alyssa A. Goodman
Email: agoodman@cfa.harvard.edu Home Page: http://cfa-www.harvard.edu/~agoodman Other information: |