email: david at ucolick.org
phone: 831-459-3281
My main research interest is centered on using moderate to
high-resolution spectroscopy to perform abundance analysis of very
metal-poor stars. These metal-poor stars act as tracers of the early
Galaxy, giving insights into the first generation of stars and
into the mechanisms that formed the Galaxy itself. By using surveys
such as the SDSS, we can
search find metal-poor stars in the Galactic halo. Following up the most promising
candidates with either moderate or high-resolution spectroscopy we can
then determine the abundances of various elements in these
stars. These abundances act like fingerprints to the processes that
created these stars, allowing us a glimpse into the early star
formation environment of the Galaxy.
Related to this, I am working on a program using the Lick
high-precision planet finding setup to monitor a sample of metal-poor
stars in an attempt to measure their companion fraction. In doing so
we hope to constrain the star formation mechanisms that can exist in
very metal-poor gas of the early Galaxy. I am also intersted in globular
clusters to both look for signs of abundance variations in individual
clusters and as labratories for how stellar evolution modifies
chemical abundances.
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