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Do Metal-rich Stars Make Metal-rich Planets? New Insights on Giant Planet Formation from Host Star Abundances This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile. † † Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory wa
Published in The Astronomical journal
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