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- W45332110 abstract "Introduction Inferring the condensation behavior of major and trace elements into SiC stardust grains in stellar environments is important for two reasons: (1) to understand the basic chemical processes that govern condensation and how they relate to the stellar environment and (2) to interpret (and predict) laboratory studies of stardust and observations of stars. Trace elements can condense in one of two ways (or some combination of them): (1) by forming grains of their own phases that are later incorporated into a major element grain or (2) by forming a solid solution with the major element phase. Even though subgrains of traceelement carbides have been observed inside graphite grains [1], our results indicate that the main condensation mechanism for trace elements is the formation of a solid solution." @default.
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- W45332110 date "2002-03-01" @default.
- W45332110 modified "2023-09-24" @default.
- W45332110 title "Condensation of Trace Elements into Presolar SiC Stardust Grains" @default.
- W45332110 hasPublicationYear "2002" @default.
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