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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.GA2025
Feedback and Star Formation Efficiency in High-Mass Star-Forming Regions
Birka Zimmermann, Stefanie Walch, Seamus D. Clarke +2
To advance our understanding of massive star formation, it is essential to perform a comprehensive suite of simulations that explore the relevant parameter space and include enough…