Table of ContentsWhat Sculpts the Interstellar Medium? Galaxies & Museums Galaxies & Museums PPT Slide Tools for finding the tools Tools for finding the tools Velocity as a "Fourth" Dimension W3 Blasting High-latitude Clouds The Velocity Field in Ursa Major Dv and vLSR Gradients PPT Slide Confirmation: Position Velocity Diagrams for H I and CO PPT Slide PPT Slide Implications of Ursa Major Study Chiseling Self-similar Structure on scales from 100 pc to 0.1 pc...in Orion Types of Line width-Size Relations ěLarsonís Lawî Scaling Relations (1981) PPT Slide Coherent Cores: ěIslands of Calm in a Turbulent Seaî Hint #1: Independent Core Rotation Hint #2: Constant Line Width in Cores? Example of the (Original) Evidence for Coherence Types of Line width-Size Relations Types of Line width-Size Relations Types of Line width-Size Relations The (Newer) Evidence for Coherence The Newest Evidence for Coherence Coherent Dense Core ěCoherenceî in Spatial Distribution of Stars The Cause of Coherence? Length Scales Relevant to Coherence Timescales Quality Control Learning More from ěToo Muchî Data The Spectral Correlation Function Goals of ěSCFî Project How the SCF Works A ěRealî Molecular Cloud Initial Comparisons using the SCF Initial Comparisons using the SCF Strong vs. Weak Field Goals of ěSCFî Project Results from SCF Project, 3/99 The Effects of Noise What Sculpts the ISM? To be discussed: Optical View of W3 Region The Velocity Field in Ursa Major |
Author: Alyssa A. Goodman
Email: agoodman@cfa.harvard.edu Home Page: cfa-www.harvard.edu/~agoodman Other information: |