Chemical signatures of planet formation in field and open cluster stars
In this thesis, I have conducted a strictly line-by-line differential abundance analysis using high resolution, high signal-to-noise ratio spectra of field stars (e.g., stellar binaries, terrestrial planet hosts etc.) and open cluster stars (e.g., the Hyades stars) in order to identify the chemical signatures of planet formation. The three main results from this thesis are: First, we present a detailed differential abundance analysis of the HAT-P-1...[Show more]
|Collections||Open Access Theses|
|Lui F Thesis 2016.pdf||1.97 MB||Adobe PDF|
Items in Open Research are protected by copyright, with all rights reserved, unless otherwise indicated.