(Q59064032)

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Properties, detectability and origin of interstellar diamonds in meteorites

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Properties, detectability and origin of interstellar diamonds in meteorites (English)

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1 reference

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Bruce T. Draine

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Edward Anders

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2

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Edward Anders

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Roy S. Lewis

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1

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English

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publication date

May 1989

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published in

Nature

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volume

339

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issue

6220

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page(s)

117-121

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https://scigraph.springernature.com/pub.10.1038/339117a0

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Interstellar Dust and Diamonds

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Interstellar diamonds in meteorites

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The size distribution of interstellar grains

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Expected particle size distributions of crystals produced from nonisothermal recrystallization

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Low-pressure, metastable growth of diamond and "diamondlike" phases

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Observational constraints on interstellar diamonds

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Peculiar ultraviolet interstellar extinction

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A search for diffuse interstellar bands in the ultraviolet

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An analysis of the shapes of ultraviolet extinction curves. II. The far-UV extinction

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Evidence for hydrogenated amorphous carbon in the Red Rectangle

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The near-infrared continuum emission of visual reflection nebulae

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Temperature fluctuations and infrared emission from interstellar grains

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Growth of Diamond Seed Crystals by Vapor Deposition

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Diamond formation in carbon-star atmospheres

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Small-particle physics and interstellar diamonds

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Formation of Xe-HL-enriched diamond grains in stellar environments

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The nature and origin of interstellar diamond

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7 January 2021

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1013731498

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(Q59064032)

Properties, detectability and origin of interstellar diamonds in meteorites

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