Formation of cosmic carbon dust analogs in partially hydrogenated atmospheres.

Details Formation of cosmic carbon dust analogs in partially hydrogenated atmospheres. Formation of cosmic carbon dust analogs in partially hydrogenated atmospheres.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996nascp3339...69b&link_type=abstract

Scientific conference: From stardust to planetesimals, p. 69 - 72

Physics

Cosmic Dust: Laboratory Simulations, Cosmic Dust: Uv Spectra

Scientific paper

The authors present UV-visible spectra of carbon grains produced by direct condensation of the carbon vapors in partically hydrogenated atmospheres. The freshly formed grains exhibit an extinction peak in the wavelength range 200 - 240 nm whose exact position depends on the hydrogen abundance. The results are discussed in terms of formation and evolution of circumstellar and interstellar cosmic dust.

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