Molecular Spectroscopy of Planet-Forming Regions in Circumstellar Disks
<p>Planets, now known to be common companions of nearby stars, are believed to originate in circumstellar disks - disks of gas and dust that form around collapsing protostars. Because of their small angular size, disks in nearby star-forming regions are difficult to spatially resolve. Howeve...
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https://thesis.library.caltech.edu/2180/12/cit_thesis.pdfhttps://thesis.library.caltech.edu/2180/1/01title.pdf
https://thesis.library.caltech.edu/2180/2/02abstract.pdf
https://thesis.library.caltech.edu/2180/3/03contents.pdf
https://thesis.library.caltech.edu/2180/4/04intro.pdf
https://thesis.library.caltech.edu/2180/5/05transdisks1.pdf
https://thesis.library.caltech.edu/2180/6/06transdisks2.pdf
https://thesis.library.caltech.edu/2180/7/07radii.pdf
https://thesis.library.caltech.edu/2180/8/08water1.pdf
https://thesis.library.caltech.edu/2180/9/09water2.pdf
https://thesis.library.caltech.edu/2180/10/10final.pdf
https://thesis.library.caltech.edu/2180/11/11bibliography.pdf
Salyk, Colette Vanessa (2009) Molecular Spectroscopy of Planet-Forming Regions in Circumstellar Disks. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/E4YF-FZ95. https://resolver.caltech.edu/CaltechETD:etd-05272009-151203 <https://resolver.caltech.edu/CaltechETD:etd-05272009-151203>