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- W3099604279 abstract "Recent ALMA observations suggest that the highest velocity part of molecular protostellar jets are launched from the dust-sublimation regions of the accretion disks ( $ 2e-6 Msun/yr) are predicted to be rich in molecules if warm (TK > 800 K). The molecular content of disk winds is very sensitive to the presence of dust and a mass-fraction of surviving dust as small as 1e-5 significantly increases the H2O and SiO abundances. Chemistry of high-velocity jets is a powerful tool to probe their content in dust and uncover their launching point. Models of internal shocks are required to fully exploit the current (sub-)millimeter observations and prepare future JWST observations." @default.
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- W3099604279 date "2020-04-17" @default.
- W3099604279 modified "2023-09-24" @default.
- W3099604279 title "Molecule formation in dust-poor irradiated jets. I. Stationary disk winds" @default.
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