Reminders Due by the end of the day: – Analysis of 10 datasets – Questions from Section 2 of Searching for and Analyzing Pulsars Tonight: I will (along.
Radar
Model Photospheres
EOS and Opacity Models in CRASH Igor Sokolov. Page 2 Our EOS and opacity functions support our UQ effort Outline –Why do we need EOS functions and opacities?
Model Photospheres I.What is a photosphere? II. Hydrostatic Equilibruium III.Temperature Distribution in the Photosphere IV. The P g -P e -T relationship.
CLUSTER SOFT EXCESS: NEW FACES OF AN OLD ENIGMA
Structured Mixed Phase of Nuclear Matter Toshiki Maruyama (JAEA) In collaboration with
A540 Review - Chapters 1, 5-10 Basic physics Boltzman equation Saha equation Ideal gas law Thermal velocity distributions Definitions Specific/mean intensities.
Stellar Evolution after the Main Sequence
Stellar Evolution
