We obtained most of the data I used in my thesis using the IRAM 30m telescope in Spain, the Haystack 37m telescope in Massachusetts, and the SEST 15m telescope in La Silla, Chile.
You can ftp each thesis chapter with the following links, the postcript files are meant to be printed on USA standard letter sized paper. All tables and figures are embedded in the text.
cover.ps.gz (14 kb)
prelim.ps.gz (24 kb)
abstract, acknowledgements, table of contents, etc.
intro.ps.gz (44 kb)
c2.ps.gz (96 kb)
"Infall Line Asymmetries in Cores with Candidate Protostars"
Contribution to the Haystack conference on Cores, Clouds and Low Mass
Stars, May 1994, ASP Conf. Ser. vol 65, page 192.
c3.ps.gz (377 kb)
"A Search for Infall Motions Toward Nearby Young Stellar Objects"
Published in 1997, ApJ, 489, 719
c4.ps.gz (1226 kb)
"Spatially Extended Motions Around Nearby Young Stellar Objects"
This is half of my thesis, it includes Appendix A with the scan maps that
didn't make it into the main text.
c5.ps.gz (311 kb)
"Radiative Transfer Models of Cores with Inward Motions"
We use a MonteCarlo spherically symmetric radiative transfer code to
explore the observed line profiles from clouds with different radial
profiles of inward speed, density, and kinetic temperature.
concl.ps.gz (18 kb)
Yes, here you will find the conclusions.
append.ps.gz (91 kb)
Appendix B is a contribution to the Maryland conference on "Star
Formation Near and Far", October 1996. Wilner, Mardones, and Myers,
"Interferometric Imaging of dense Gas Tracers in the Protostellar
Candidate L1527," in AIP CP 393, page 109.
Appendix C has many of the standard equations to determine column
densities etc from mm-wavelength molecular lines.
Appendix D talks about the antenna radiation pattern and the
observable temperature scale from a single dish radio telescope.