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Silicon carbide and the origin of interstellar carbon grains

scientific article published in Nature

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title

Silicon carbide and the origin of interstellar carbon grains (English)

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1 reference

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E. D. Feigelson

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M. Frenklach

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1

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C. S. Carmer

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2

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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

6221

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page(s)

196-198

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exact match

https://scigraph.springernature.com/pub.10.1038/339196a0

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Optical properties of interstellar graphite and silicate grains

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Interstellar Dust and Diamonds

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Space, Stars, C60, and Soot

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Infrared spectroscopy over the 2.9-3.9 mu.m. waveband in biochemistry and astronomy

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Formation and flow of dust grains in cool stellar atmospheres

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Dust and molecules in the shells of carbon stars - the inverse greenhouse effect

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Composition of Interstellar Grains

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High-resolution spectra of cool stars in the 10- and 20-micron regions

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2-14 mu m stellar spectrophotometry. I. Stars of the conventional spectral sequence

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

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The IRC +10216 circumstellar envelope. II. Spatial measurements of the dust

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Evidence for interstellar SiC in the Murray carbonaceous meteorite

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Large isotopic anomalies of Si, C, N and noble gases in interstellar silicon carbide from the Murray meteorite

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10.1038/339196A0

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1000108154

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(Q58995413)

Silicon carbide and the origin of interstellar carbon grains

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