{"id":{"repo_id":"uiuc","oai_identifier":"oai:www.ideals.illinois.edu:2142/85168"},"canonical_url":"https://search.dev.ndltd.org/etd/uiuc/oai:www.ideals.illinois.edu:2142/85168","repository":{"repo_id":"uiuc","name":"University of Illinois - Urbana-Champaign","base_url":"https://www.ideals.illinois.edu/oai-pmh"},"display":{"title":"Interferometric Mapping of Magnetic Fields in Star -Forming Regions","abstract":"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.","abstract_html":"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. 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