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- W1409968684 abstract "Context. Gas plays a major role in the dynamical evolution of protoplanetary discs. Its coupling with the dust is the key to our understanding of planetary formation. Studying the gas content is therefore a crucial step towards understanding protoplanetary discs evolution. Such a study can be made through spectroscopic observations of emission lines in the FIR, where some of the most important gas coolants emit, such as the [OI] 3P1 → 3P2 transition at 63.18 μm." @default.
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- W1409968684 date "2015-02-13" @default.
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- W1409968684 title "Herschel-PACS observations of [OI] and H2O in Chamaeleon II" @default.
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