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- W2893668862 abstract "Condensation of circumstellar dust begins with formation of molecular clusters close to the stellar photosphere. These clusters are predicted to act as condensation cores at lower temperatures and allow efficient dust formation farther away from the star. Recent observations of metal oxides, such as AlO, AlOH, TiO, and TiO$_2$, whose emission can be traced at high angular resolutions with ALMA, have allowed first observational studies of the condensation process in oxygen-rich stars. We are now in the era when depletion of gas-phase species into dust can be observed directly. I review the most recent observations that allow us to identify gas species involved in the formation of inorganic dust of AGB stars and red supergiants. I also discuss challenges we face in interpreting the observations, especially those related to non-equilibrium gas excitation and the high complexity of stellar atmospheres in the dust-formation zone." @default.
- W2893668862 created "2018-10-05" @default.
- W2893668862 creator A5079430031 @default.
- W2893668862 date "2018-09-27" @default.
- W2893668862 modified "2023-10-16" @default.
- W2893668862 title "Molecular dust precursors in envelopes of oxygen-rich AGB stars and red supergiants" @default.
- W2893668862 hasPublicationYear "2018" @default.
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