Table of ContentsWatching the Interstellar Medium Move Bart Bok and the ėDark Nebulaeî PPT Slide Taurus Dark Cloud Complex 100 mm ISSA image Taurus: Star Counting Taurus: Star Counting, Color Excess of Stars Taurus: All Methods of Measuring Extinction Bart Bok in 1955 Adding a Third Dimension PPT Slide Watching the ISM Move W3 The Origin and Evolution of High-Latitude Clouds 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 PPT Slide Bok and his Globules Bok and his Globules 1990: ėBart Bok Was Correct!î Motions Of, In and Around Dense Cloud Cores Coherent Cores: ėIslands of Calm in a Turbulent Seaî Hint #1: Independent Core Rotation Hint #2: Constant Line Width in Cores? Types of Line width-Size Relations Types of Line width-Size Relations Types of Line width-Size Relations Types of Line width-Size Relations An Example of the (Original) Evidence for Coherence The (Newer) Evidence for Coherence Coherent Dense Core ėCoherenceî in Spatial Distribution of Stars The Cause of Coherence? Learning More from ėToo Muchî Data The Spectral Correlation Function Goals of ėSCFî Project How the SCF Works A ėRealî Molecular Cloud Initial Comparisons using the SCF Initial Comparisons using the SCF Goals of ėSCFî Project Watching the ISM Move Next section contains "optional" slides, not used. Optical View of W3 Region ėGo no further than AV~1.3 mag.î ėStar and Planet Formationî The Velocity Field in Ursa Major |
Author: Alyssa A. Goodman
Email: agoodman@cfa.harvard.edu Home Page: cfa-www.harvard.edu/~agoodman Other information: |