U & Th Decay Series Isotope Geochemistry Lecture 33.
Lecture 3: Experimental measurements ( chpt 5, Feynman)
1 THE LOCAL HIGH REDSHIFT UNIVERSE – THE EXTREMELY METAL POOR STARS IN THE GALACTIC HALO Why study very metal poor stars ? We can study the early epochs.
How Many SN Contribute to an EMP Star’s Chemical Inventory ?
Lecture 3: Experimental measurements (chpt 5, Feynman)
