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• W3161635484 endingPage "A173" @default.
• W3161635484 startingPage "A173" @default.
• W3161635484 abstract "We present SOFIA/FIFI-LS observations of three Class 0 and one Class I outflows (Cep E, HH 1, HH 212, and L1551 IRS5) in the far-infrared [O I]63mum and [O I]145mum transitions. Spectroscopic [O I]63mum maps enabled us to infer the spatial extent of warm, low-excitation atomic gas within these protostellar outflows. If proper shock conditions prevail, the instantaneous mass-ejection rate is directly connected to the [O I]63mum luminosity. In order to unravel evolutionary trends, we analysed a set of 14 Class 0/I outflow sources that were spatially resolved in the [O I]63mum emission. We compared these data with a sample of 72 Class 0/I/II outflow sources that have been observed with Herschel (WISH, DIGIT, WILL, GASPS surveys) without spatially resolving the [O I]63mum line." @default.
• W3161635484 created "2021-05-24" @default.
• W3161635484 creator A5001560798 @default.
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• W3161635484 creator A5051339347 @default.
• W3161635484 creator A5061044084 @default.
• W3161635484 creator A5065189238 @default.
• W3161635484 date "2021-06-01" @default.
• W3161635484 modified "2023-10-16" @default.
• W3161635484 title "Evolution of the atomic component in protostellar outflows" @default.
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