Dust Formation Chemistry in Carbon-Rich Wolf-Rayet Winds

Details Dust Formation Chemistry in Carbon-Rich Wolf-Rayet Winds Dust Formation Chemistry in Carbon-Rich Wolf-Rayet Winds

Jul 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997ap%26ss.251..389l&link_type=abstract

Astrophysics and Space Science, Volume 251, Issue 1-2, pp. 389-392

Astronomy and Astrophysics

Astrophysics

Scientific paper

Dust formation processes are investigated in the hot hydrogen-deficient
wind of carbon-rich Wolf-Rayet (WC) stars. Results show that dust
precursors (small linear carbon chains) form in large quantities only at
high gas densities. This suggests that a clumpy wind or an equatorial
disc are necessary to trigger dust formation in WC stars.

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