Abstract
Only a very small fraction of interstellar dust mass originates within the cooling expansions of supernova interiors; but those solids are exciting and important for other reasons. Thermally condensed (high-T) solids that do originate in this way may provide the refractory cores of a significant fraction of interstellar medium (ISM) grains. Hoyle & Wickramasinghe (1970) had predicted this source of grains. Clayton (1975a, 1975b) introduced the possibility of finding such grains in meteorites through their isotopic peculiarities, which were inherited during condenstaion within young supernova ejecta. Such thermally condensed cores within expanding supernova interiors were designated by the acronym SUNOCON by Clayton (1978) as a specific scientific name for such objects. The discovery of these grains, preserved within the meteorites from the beginnings of the solar system and now studied in high detail in laboratories, is the topic of this paper.
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Clayton, D.D., Amari, S., Zinner, E. (1997). Dust from Supernovae. In: Cherchneff, I., Millar, T.J. (eds) Dust and Molecules in Evolved Stars. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-1307-8_57
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DOI: https://doi.org/10.1007/978-94-017-1307-8_57
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