62 citations · 1k across the 43 of their papers we have counts for
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Compressed magnetic field in the magnetically-regulated global collapsing clump of G9.62+0.19
Tie Liu, Kee-Tae Kim, Sheng-Yuan Liu +22
How stellar feedback from high-mass stars (e.g., H{\sc ii} regions) influences the surrounding interstellar medium and regulates new star formation is still unclear. To address thi…
A Submillimeter Burst of S255IR~SMA1 - The Rise And Fall Of Its Luminosity
Sheng-Yuan Liu, Yu-Nung Su, Igor Zinchenko +2
Temporal photometric variations at near infrared to submillimeter wavelengths have been found in low-mass young stellar objects. These phenomena are generally interpreted as accret…
Disks and outflows in the S255IR area of high mass star formation from ALMA observations
I. Zinchenko, S. -Y. Liu, Y. -N. Su +1
We describe the general structure of the well known S255IR high mass star forming region, as revealed by our recent ALMA observations. The data indicate a physical relation of the…
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…