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Possible Counter Rotation between the Disk and Protostellar Envelope around the Class I Protostar IRAS 04169+2702
Shigehisa Takakuwa, Yusuke Tsukamoto, Kazuya Saigo +1
We present results from our SMA observations and data analyses of the SMA archival data of the Class I protostar IRAS 04169+2702. The high-resolution (~0.5") CO (3-2) image…
Polarization Properties and Magnetic Field Structures in the High-Mass Star-Forming Region W51 Observed with ALMA
Patrick M. Koch, Ya-Wen Tang, Paul T. P. Ho +3
We present the first ALMA dust polarization observations towards the high-mass star-forming regions W51 e2, e8, and W51 North in Band 6 (230 GHz) with a resolution around 0.26" ($\…
Magnetic Fields from Filaments to Cores
Patrick M. Koch, Ya-Wen Tang, Nicholas L. Chapman +7
How important is the magnetic (B-) field when compared to gravity and turbulence in the star-formation process? Does its importance depend on scale and location? We summarize submm…