X-RAY INTERACTION WITH MATTER. COLLIMATE OR NOT TO COLLIMATE?! SCATTER.
Stars & The Sun If you want to make an apple pie from scratch, you must first create the Universe- Carl Sagan.
The Collective Model Aard Keimpema. Contents Vibrational modes of nuclei Deformed nuclei Rotational modes of nuclei Coupling between rotational and vibrational.
1. accretion disk - flat disk of matter spiraling down onto the surface of a star. Often from a companion star.
Simulation Parameters and Results We performed nine simulations to test the sensitivity of our results to resolution, viscous stress-to-pressure ratio.
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 % (
Development of Giant Air Shower in Earth’s Atmosphere.
Lecture 2: Formation of the chemical elements Bengt Gustafsson: Current problems in Astrophysics Ångström Laboratory, Spring 2010.
AGASA results Anisotropy of EHE CR arrival direction distribution
Study of high energy cosmic rays with the sparse very large air shower array ALTA/CZELTA
The Evolution and Explosion of Massive Stars Nuclear Physics Issues
Die Mesonproduktion
