Can Photo-Evaporation Trigger Planetesimal Formation? Henry Throop John Bally SWRI Univ.Colorado / CASA DPS 12-Oct-2004.
Spine Outline Sports Med. Anatomy Bones of the Vertebral Column Bones of the Vertebral Column 33 vertebrae 33 vertebrae 24 movable (true) 24 movable (true)
© 2004 Pearson Education Inc., publishing as Addison-Wesley Star Stuff.
AST101 The Evolution of Galaxies. Virgo Cluster Collisions of Galaxies Outside of Clusters (the field), most galaxies are spiral or irregular In dense.
Time space Cosmic bullet temperature. Another look at dark halos J. Dubinski Toronto/CITA New big cosmo simulations Halos vs. Elliptical Galaxies –deVaucouleurs.
The orbits of the planets - A clue to the formation of our Solar System All planets orbit the sun in the same direction. Most rotate in this direction.
Failure Correction Techniques for Large Disk Array
GALAXIES. There are Three main classes (as classified by Hubble). A. Spiral B. Elliptical C. Irregular 1. Spiral galaxies. Disk + central bulge. M51 M51.
THE BIRTH OF THE SOLAR SYSTEM. MODELS OF THE SOLAR SYSTEM Geocentric - Everything revolved around earth. (Aristotle and Ptolemy) Heliocentric – Planets.
Beyond Our Solar System: The Search for Extrasolar Planetary Systems Produced by and for the Outreach Lecture Series of the Environmental Science Institute.
The Milky Way Disk and the LAMOST survey Jinliang HOU Shanghai Astronomical Observatory, CAS Workshop on Galactic Studies with the LAMOST Survey KIAA-PKU,
1 Failure Correction Techniques for Large Disk Array Garth A. Gibson, Lisa Hellerstein et al. University of California at Berkeley.
