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University of Illinois at Urbana-Champaign

Interferometric Mapping of Magnetic Fields in Star -Forming Regions

Abstract

dc:description

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.

Degree

thesis:*
Name thesis:degree_name
Ph.D.
Level thesis:degree_level
Dissertation
Discipline thesis:degree_discipline
Astronomy
Grantor
University of Illinois at Urbana-Champaign
Year dc:date
2015

Author and committee

dc:creator, dc:contributor.*
Author dc:creator
  • Lai, Shih-Ping
Contributors dc:contributor
  • Lewis Snyder

Subjects

dc:subject × 1

Rights

Language dc:language
eng

Identifiers

dc:identifier.*
Identifier
(MiAaPQ)AAI3023106
OAI identifier oai:identifier
oai:www.ideals.illinois.edu:2142/85168

Chain of custody

source
Harvested from
University of Illinois - Urbana-Champaign
Base URL
www.ideals.illinois.edu/oai-pmh
Last updated
2026-07-22
Source record
OAI-PMH GetRecord
citation

Lai, Shih-Ping. Interferometric Mapping of Magnetic Fields in Star -Forming Regions. Dissertation thesis, University of Illinois at Urbana-Champaign, 2015. http://hdl.handle.net/2142/85168