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• W3099687850 abstract "Context. Understanding how protostars accrete their mass is one of the fundamental problems of star formation. High dust column densities and complex kinematical structures make direct observations challenging. Moreover, direct observations only provide a snapshot. Chemical tracers provide an interesting alternative to characterise the infall histories of protostars." @default.
• W3099687850 created "2020-11-23" @default.
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• W3099687850 date "2016-10-26" @default.
• W3099687850 modified "2023-10-15" @default.
• W3099687850 title "Water around IRAS 15398–3359 observed with ALMA" @default.
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• W3099687850 doi "https://doi.org/10.1051/0004-6361/201628795" @default.
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