Riunione Avanzamento 1 ASI – Roma 11 Novembre 2008 INAF IFSI IRA OAFI OACT UNIRM1 UNIRM2 UNILE 1 SWG3: Evolution of Young Stellar Objects Goals Establish.
D EBRIS DISKS WITH H ERSCHEL : AN OVERVIEW OF THE DUNES MODELING ACTIVITIES Jean-Charles Augereau, Steve Ertel, Alexander Krivov, Jérémy Lebreton, Torsten.
ExoZodiacal Emission and Challenge and Opportunity for The Detection of ExoPlanets C. Beichman Friday, March 26, 2010 5 AU Workshop With lots of help from.
Cold dust in the Galactic halo: first detection of dust emission in a high-velocity cloud : Francois Boulanger et Marc-Antoine Miville-Deschênes Miville.
Emil-Christensen-SASP-2014
Visible Light and Beyond “White light” is made up of a rainbow of colors, each with a different wavelength.
SN 1987A the excitement continues Bruno Leibundgut ESO.
[email protected]. Last Version: DR3.5 Released June 2012 Pipeline: Optimised De- glitcher BriGAdE Allow Dark Pixel drift removal.
William Herschel
Milky Way
ALMA During Early Science National Radio Astronomy Observatory - NAASC Charlottesville, Virginia.
Measurement of the Relative Abundances of the Ultra-Heavy Galactic Cosmic-Rays (30 Z 40) with TIGER Washington University in St. Louis B.F. Rauch,
