GeoSoilEnviroCARS, The University of Chicago 16-Oct-2005 Matt Newville, Steve Sutton, Mark Rivers, Peter Eng Consortium for Advanced Radiation Sources.
Abundances and relation to PN morphological features Antonio Mampaso IAC, Tenerife. Spain.
Stars science questions Origin of the Elements Mass Loss, Enrichment High Mass Stars Binary Stars.
METEORITES. METEORITE COMPOSITION 93% Stony Meteorites: Fe, Mg, Si, O compounds as oxides and silicates 6% Iron Meteorites: Fe-Ni alloys 1% Chondrites:
THE BIG DIP experimental and systematic discussions of neutron binding in very neutron-rich nuclides William B. Walters Department of Chemistry University.
Compilation of stellar fundamental parameters from literature : high quality observations + primary methods Calibration stars for astrophysical parametrization.
Announcements Pick up graded homework (projects, tests still in progress) Transit of Mercury (crossing in front of Sun), this afternoon, roughly noon-5:00.
Infrared Spectroscopy of Neutron-Capture Elements in Planetary Nebulae N. C. Sterling & H. L. Dinerstein ABSTRACT We present results from an ongoing survey.
Low Temperature X-ray Detectors Caroline K. Stahle NASA / Goddard Space Flight Center.
The Structure of the Solar Atmosphere Hugh Hudson UC Berkeley and University of Glasgow.
Studying GRB Environments and Progenitors with Absorption Spectroscopy
Lecture 2 Abundances. Any study of nucleosynthesis must have one of its key objectives an accurate, physically motivated explanation for the pattern of.