Bologna 22.01.2009 The size evolution of early-type galaxies since z=2 P. Saracco1, M. Longhetti1, with the contribution of S. Andreon1, A. Mignano1, G. Feulner 2, N. Drory…

The Formation and Structure of Stars Chapter 9 0 The Interstellar Medium (ISM) Gas: ~75% H, 25% He, traces of “metals” 1% “dust” (silicates, carbon, heavy elements…

Assimilation GPS Radio Occultation Data in a GSI framework Impact of Infrared, Microwave and Radio Occultation Satellite Observations on Operational Numerical Weather Prediction…

A Search for Quiet Massive X-Ray Binaries M. Virginia McSwain Yale University Tabetha S. Boyajian Erika Grundstrom Douglas R. Gies Georgia State University A Quiet Massive…

Ge/Ay133 What can transit observations tell us about (exo)-planetary science? Sometimes the absence of signal is interesting: No transits in 47 Tuc, `expectationâ=30-40…

Ge/Ay133 What can transit observations tell us about (exo)-planetary science? Part II – “Spectroscopy” & Atmospheric Composition/Dynamics Kudos to Heather Knutson,…

Star-Forming Galaxies and the IGM in the z=1.5-2.5 “Redshift Desert” C. Steidel, D. Erb, N. Reddy (Caltech) A. Shapley (Berkeley) M. Pettini (IoA, Cambridge) K. Adelberger…

Nearby Galaxies (mostly) at mm and IR wavelengths Adam Leroy (MPIA Heidelberg) Christof Buchbender (IRAM Granada) Liberally plundering .ppt by: Eric Bell, Hans-Walter Rix,…