Phoenix Lander lands at the pole on Sunday !! Admin Review lecture today (and posted on the web) Final Exam:  10:30am May 28th (Wednesday), SHL 131 1, 2, 3, 4, 5, 10,…

Slide 1 Slide 2 LISA A Mission to detect and observe Gravitational Waves O. Jennrich, ESA/ESTEC on behalf of the LISA Science Team Slide 3 LISA 2 Réunion LISA-France, Collège…

Slide 1PI: Michele Cirasuolo Royal Observatory Edinburgh Collaborators: J. Dunlop, R. McLure, F. Cullen, R. Maiolino, R. Ivison, G. Wright, M. Swinbank, R. Sharples, R. Bower,…

Slide 1http://chandra.h arvard.edu/phot o/2007/m51/ Slide 2 Confronting Stellar Feedback Simulations with Observations of Hot Gas in Elliptical Galaxies Q. Daniel Wang, Shikui…

Slide 1Magnetic dynamos in accretion disks Magnetic helicity and the theory of astrophysical dynamos Dmitry Shapovalov JHU, 2006 Slide 2 Outline - Turbulence and magnetic…

Slide 1Astronomical Wide-field Imaging System for Europe MPE/USM Survey/GTO Projects Mark Neeser MPE / ESO Mark Neeser MPE / ESO Leiden Workshop Nov. 2005 Slide 2 MPE/USM…

1. The Astrophysical Journal, 772:110 (16pp), 2013 August 1 doi:10.1088/0004-637X/772/2/110 C 2013. The American Astronomical Society. All rights reserved. Printed in the…

1. The Hidden Mass and Large Spatial Extent of a Post-Starburst Galaxy Outflow Todd M. Tripp, et al. Science 334, 952 (2011); DOI: 10.1126/science.1209850 This copy is for…

Slide 1COSMIC MAGNETIC FIELDS ElisaBete M. de Gouveia Dal Pino IAG-USP UFRRJ, October 2005 Slide 2 PREAMBLE Most of visible matter in the Universe is in plasma state: composed…

Slide 1Type Ia Supernovae Progenitors Slide 2 Type Ia Supernovae Historical defining characteristics: Generally, lack of lines of hydrogen Contain a strong Si II absorption…