Condensation and growth of hydrogenated carbon clusters in carbon-rich stars }

Details Condensation and growth of hydrogenated carbon clusters in carbon-rich stars } Condensation and growth of hydrogenated carbon clusters in carbon-rich stars }

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000a%26a...359..799p&link_type=abstract

Astronomy and Astrophysics, v.359, p.799-810 (2000)

Astronomy and Astrophysics

Astrophysics

13

Molecular Processes, Stars: Circumstellar Matter, Ism: General, Ism: Molecules

Scientific paper

Hydrogenated carbon cluster growth in carbon-rich stellar atmospheres is simulated by a model which takes into account the simultaneous formation of carbon compounds with carbon atoms under various states of hybridization. A grid of computations shows that a mixture of different species can appear (small hydrogenated carbon clusters, carbon chains or ring-shaped structures, aromatic-like entities, etc.) depending on both carbon to hydrogen relative abundance and temperature of the star. Dehydrogenation rate and sp2/sp and sp3/sp ratios are estimated.

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