Dense clumps in NGC 2024 — Protostellar condensations?
作者： A. Schulz , R. Zylka , R. Güsten
DOI: 10.1007/BFB0114854
关键词: Resolution (electron density) 、 Orion Nebula 、 Interstellar medium 、 Physics 、 Continuum (design consultancy) 、 Molecular cloud 、 Protostar 、 Astrophysics 、 Astronomy 、 Excitation 、 Star formation
摘要: We performed a multi-line NH 3 and CS excitation study with the highest possible single-dish resolution to analyze temperature density structure of NGC 2024 molecular cloud core. A physically consistent picture is presented that matches both presently available line dust continuum data
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