Pop III IMF Michael L. Norman Laboratory for Computational Astrophysics UC San Diego (with thanks to Andrea Ferrara & Mario Livio)
IRAC/MIPS view of the ISM: PAHs dominate in IRAC Li & Draine (2001) dust emissivity model; only very strong (> 10 3 x avg.) radiation fields contribute.
Part I Properties and Origins of Long GRBs. The Origin of Long-Period GRBs Knicole Colón High Energy Astrophysics March 5, 2008.
Type Ia supernovae and the ESSENCE supernova survey Kevin Krisciunas.
Supernovae Lab 9. Let’s go Supernova! Stars which are ≥ 8x massive than our Sun end their lives in a most spectacular way; they go supernova! First, the.
