2 papers
astro-ph.GA2025
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…
astro-ph.GA2024
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…