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The 0Z Project


The 0Z project is a large observational program to more than double the number of extremely metal poor stars with high dispersion abundance analyses, with the aim of shedding light on the early epoch of the formation of the Galaxy, the chemical evolution of the Galaxy, and related issues. This is being accomplished by observing candidate stars from the Hamburg/ESO Survey (HES) (which has a two times higher effective yield of extremely metal poor stars than the existing HK survey) with Keck I/HIRES, and, starting in 2002, also with Magellan 1.



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Last modified: Wed Oct 17 15:07:27 CEST 2001