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astro-ph.GA2026
HINSPHERES: Spherically Symmetric Radiative Transfer Modeling of HINSA and the Radial HI-to-H Transition in Molecular Clouds
Yuchen Xing, Di Li, Xin Lyu +10
The transition from atomic hydrogen (HI) to molecular hydrogen (H) is the first step in the evolution from diffuse interstellar gas to dense star-forming cores. HI narrow self-…
astro-ph.GA2026
Identifying the principal mechanism of star formation feedback
Chong Li, Rouyu Li, Keping Qiu +27
Feedback from massive stars regulates the formation of next-generation stars and planets and thus shapes the evolution of galaxies, yet observational evidence capable of determinin…