tipa -- 11/4/2010

Common origin for radio relics and halos: galaxy cluster-wide, homogeneous cosmic-ray distribution, and evolving magnetic fields

• Authors: Uri Keshet

Using the X-ray Morphologies of Young Supernova Remnants to Constrain Explosion Type, Ejecta Distribution, and Chemical Mixing

• Authors: Laura A. Lopez (UCSC), Enrico Ramirez-Ruiz (UCSC), Daniela Huppenkothen (Amsterdam), Carles Badenes (Tel-Aviv, Weizmann Institute of Science), David Pooley (Eureka)

Population I Wolf-Rayet Runaway Stars: the Case of WR124 and its Expanding Nebula M1-67

• Authors: S.V. Marchenko, A.F.J. Moffat, P.A. Crowther

Constraints on the Cosmic-Ray Density Gradient beyond the Solar Circle from Fermi gamma-ray Observations of the Third Galactic Quadrant

• Authors: Fermi LAT Collaboration

Assessing Radiation Pressure as a Feedback Mechanism in Star-Forming Galaxies

• Authors: Brett H. Andrews, Todd A. Thompson

p, He, and C to Fe cosmic-ray primary fluxes in diffusion models: Source and transport signatures on fluxes and ratios

• Authors: A. Putze, D. Maurin, F. Donato