tipa -- 3/30/2016

The Efficiency of B-Field Amplification at Shocks by Turbulence

• Suoqing Ji, S. Peng Oh, Mateusz Ruszkowski, Maxim Markevitch

Numerical Modeling of the Early Light Curves of Type IIP Supernovae

• Viktoriya Morozova, Anthony L. Piro, Mathieu Renzo, Christian D. Ott

A burst in a wind bubble and the impact on external matter: high-energy gamma-ray flares and implications for fast radio bursts and pulsar-driven supernovae

• Kohta Murase, Kazumi Kashiyama, Peter Meszaros

The repeating Fast Radio Burst FRB 121102: Multi-wavelength observations and additional bursts

• P. Scholz, L. G. Spitler, J. W. T. Hessels, S. Chatterjee, J. M. Cordes, V. M. Kaspi, R. S. Wharton, C. G. Bassa, S. Bogdanov, F. Camilo, F. Crawford, J. Deneva, J. van Leeuwen, R. Lynch, E. C. Madsen, M. A. McLaughlin, M. Mickaliger, E. Parent, C. Patel, S. M. Ransom, A. Seymour, I. H. Stairs, B. W. Stappers, S. P. Tendulkar