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The Magnetic Field in the Class 0 Protostellar Disk of L1527
Dominique M. Segura-Cox, Leslie W. Looney, Ian W. Stephens +5
We present subarcsecond (~0.35") resolved observations of the 1.3 mm dust polarization from the edge-on circumstellar disk around the Class 0 protostar L1527. The inferred magnetic…
Testing Magnetic Field Models for the Class 0 Protostar L1527
J. A. Davidson, Z. -Y. Li, C. L. H. Hull +10
For the Class 0 protostar, L1527, we compare 131 polarization vectors from SCUPOL/JCMT, SHARP/CSO and TADPOL/CARMA observations with the corresponding model polarization vectors of…
Spatially Resolved Magnetic Field Structure in the Disk of a T Tauri Star
Ian W. Stephens, Leslie W. Looney, Woojin Kwon +6
Magnetic fields in accretion disks play a dominant role during the star formation process but have hitherto been observationally poorly constrained. Field strengths have been infer…
Spitzer Observations of Dust Emission from HII Regions in the Large Magellanic Cloud
Ian W. Stephens, Jessica Marie Evans, Rui Xue +3
Massive stars can alter physical conditions and properties of their ambient interstellar dust grains via radiative heating and shocks. The HII regions in the Large Magellanic Cloud…