Publication Date:
2019-08-17
Description:
This paper evaluates the condensation of carbon solids in a gas of pure C and O atoms when these exist within the interior of an expanding young supernova. We calculate the abundances of large carbon molecules, which serve as nucleations for condensation of graphites. Additional information is contained in the original extended abstract.
Keywords:
Lunar and Planetary Science and Exploration
Type:
Lunar and Planetary Science XXXII; LPI-Contrib-1080
Format:
text
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