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oai:www.ideals.illinois.edu:2142/85168 2023-07-11 col_2142_5131 col_2142_14807 com_2142_5130 com_2142_14806 com_2142_8903

Lewis Snyder Lai, Shih-Ping 2015-09-25T22:35:34Z 2015-09-25T22:35:34Z 10000-01-01 2001 2001 In addition, it is generally found in my sample that the degree of dust polarization decreases toward the high intensity regions and toward the center of the core. These results suggest that the dust polarization efficiency decreases toward the regions with high density and/or high optical depth. Made available in DSpace on 2015-09-25T22:35:34Z (GMT). No. of bitstreams: 2 license.txt: 4848 bytes, checksum: 96035ab3f5e1c23cc7138a224ce498bd (MD5) 3023106.pdf: 4698035 bytes, checksum: 16d7b3e766d74b8b1223ff3a3920a3a2 (MD5) Previous issue date: 2001 Embargo set by: Seth Robbins for item 86449 Lift date: Forever Reason: Restricted to the U of I community idenfinitely during batch ingest of legacy ETDs Restricted to the U of I community idenfinitely during batch ingest of legacy ETDs U of I Only 94 p. Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2001. http://hdl.handle.net/2142/85168 (MiAaPQ)AAI3023106 eng Physics, Astronomy and Astrophysics Interferometric Mapping of Magnetic Fields in Star -Forming Regions text Astronomy Astronomy University of Illinois at Urbana-Champaign Dissertation Ph.D.