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oai:www.ideals.illinois.edu:2142/85180 2023-07-11 col_2142_5131 col_2142_14807 com_2142_5130 com_2142_14806 com_2142_8903

Crutcher, Richard M. Cortes, Paulo Cesar 2015-09-25T22:35:37Z 2015-09-25T22:35:37Z 10000-01-01 2005 2005 We developed a code to model and observe the polarized dust emission from arbitrary magnetic field configurations in star forming regions. We found that the interferometric observation will strongly overestimate the fractional polarization under most cases; however, we found that the position angle is preserved with errors that are in the range of observable quantities. Made available in DSpace on 2015-09-25T22:35:37Z (GMT). No. of bitstreams: 2 license.txt: 4848 bytes, checksum: 96035ab3f5e1c23cc7138a224ce498bd (MD5) 3202080.pdf: 3610208 bytes, checksum: aa081062702c7933a83b9c413be1ffb0 (MD5) Previous issue date: 2005 Embargo set by: Seth Robbins for item 86461 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 135 p. Thesis (Ph.D.)--University of Illinois at Urbana-Champaign, 2005. http://hdl.handle.net/2142/85180 (MiAaPQ)AAI3202080 eng Physics, Astronomy and Astrophysics Magnetic Fields in Star Forming Regions: Interferometric Mapping and Modeling text Astronomy Astronomy University of Illinois at Urbana-Champaign Dissertation Ph.D.