Non xrays from_the_very_nearby_typeia_sn_2014j_constraints_on_its_environment
Multi dimensional simulations_of_the_expanding_supernova_remnant_of_sn1987_a
The s-process Fe Co Ni Rb Ga Ge Zn Cu Se Br As Zr Y Sr Kr (n, ) ()() ()() r-process p-process 63 Ni, t 1/2 =100 a 64 Cu, t 1/2 =12 h, 40 % (
Takaaki Kajita ICRR, Univ. of Tokyo
Charge Exchange Models for X-ray Spectroscopy with AtomDB v2.0
ADVANCED CONCEPT FOR HIGH ENERGY ACCELERATOR