Kinematics of the Ursa Major Molecular Clouds

A Web Site for the Paper which appeared in the Astrophysical Journal, June 10, 1997

 Marc W. Pound

Radio Astronomy Laboratory, University of California, Berkeley, CA 94720

pound@teddi.berkeley.edu

Alyssa A. Goodman

Department of Astronomy Harvard University Cambridge, MA 02138

agoodman@cfa.harvard.edu


This page provides the Abstract of our paper as an image (below), and links to all of the Figures in the paper. Those of you desirous of a POSTSCRIPT files of the text and figures, should ftp all the files at ftp://cfa-ftp.harvard.edu/ftp/pub/agoodman/Ursa/preprint/ The files ending in .cps are COLOR.

All of the Figures can be accessesed as jpeg files, indexed with the numbers used in list, below.

List of Figures:

  1. IRAS 100-micron flux-density image of NCP Loop.
  2. Zoom of 100-micron map to just Ursa Major Clouds, with background subtracted.
  3. 100-micron opacity in Ursa Major
  4. Dust Temperature in Ursa Major
  5. Integrated CO Map of Ursa Major
  6. Schematic Finding Chart for Ursa Major Clouds
  7. Channel Maps of CO in Ursa Major (Part 1, Part 2, Part 3)
  8. Filaments in Ursa Major, CO (Part 1, Part 2)
  9. Arcs at the Filament Tips, CO
  10. Map of CO centroid velocity (color)
  11. Kinematic Properties of atomic and molecular gas as a function of b
  12. Integrated H I intensity and sample spectra
  13. Map of HI centroid velocity (color)
  14. HI velocity field inside and outside the Ursa Major Filament
  15. Position Velocity Diagrams for HI and CO in Ursa Major
  16. Centroid Velocity Differences (CO-HI) as a Function of Position
  17. Cartoon Model of Ursa Major System
  18. Model for NCP Loop Expansion and Ursa Major Clouds
  19. Explanation of the gradients seen in HI
  20. Cuts showing correlation of magnetic field strength with column density along filament

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