22 citations · 22 across the 4 of their papers we have counts for
4 papers
Can Clump Properties Predict Core Distribution in Star Formation? A Statistical Analysis of MHD Simulations
Wei-An Chen, Seamus D. Clarke, Ya-Wen Tang
Dense cores, the progenitors of stars, are in sub-pc scale and fragmented from pc-scale clumps. However, it is still unclear that how strongly the fragmentation process is affected…
Alignment Parameters: Quantifying Dense Core Alignment in Star-forming Regions
Wei-An Chen, Ya-Wen Tang, Seamus D. Clarke
Recent high-resolution observations at millimeter (mm) and sub-mm reveal a diverse spatial distribution for sub-pc scale dense cores within star-forming regions, ranging from clust…
New Insights on 30 Dor B Revealed by High-Quality Multi-wavelength Observations
Wei-An Chen, Chuan-Jui Li, You-Hua Chu +4
The supernova remnant (SNR) 30 Dor B is associated with the \ion{H}{2} region ionized by the OB association LH99. The complex interstellar environment has made it difficult to stud…
Formation of the SDC13 Hub-Filament System: A Cloud-Cloud Collision Imprinted on The Multiscale Magnetic Field
Jia-Wei Wang, Patrick M. Koch, Ya-Wen Tang +6
Hub-filament systems (HFSs) are potential sites of protocluster and massive star formation, and play a key role in mass accumulation. We report JCMT POL-2 850 m polarization obs…