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Abundances of Linear Carbon-Chain Molecules in SupernovaeThis 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.
Document ID
20010044846
Acquisition Source
Headquarters
Document Type
Abstract
Authors
Clayton, D. D. (Clemson Univ. SC United States)
Deneault, E. (Clemson Univ. SC United States)
Meyer, B. S. (Clemson Univ. SC United States)
The, L.-S. (Clemson Univ. SC United States)
Date Acquired
August 20, 2013
Publication Date
January 1, 2001
Publication Information
Publication: Lunar and Planetary Science XXXII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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