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from Part II - Low-Mass Star Formation (LMSF)
Published online by Cambridge University Press: 11 April 2023
Through the emission observations of molecular species in the IRAS2 and IRAS4 locations in NGC 1333 in the Perseus Molecular Cloud (PMC), the distinctions between conditions favouring COMs or WCCC production in the immediate neighbourhoods of low-mass protostars are discussed. The current chemical modelling and that which will follow from accumulating higher-resolution observations using the latest generation of millimetre and submillimetre instrumentation are discussed.
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