Condensed carbon in white dwarf atmospheres

Details Condensed carbon in white dwarf atmospheres Condensed carbon in white dwarf atmospheres

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983pazh....9..227z&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 9, Apr. 1983, p. 227-229) Soviet Astronomy Letters (ISSN 0360-0327), vol. 9, Mar.-Apr.

Astronomy and Astrophysics

Astronomy

1

Carbon, Condensing, Stellar Atmospheres, Stellar Models, White Dwarf Stars, Abundance, Graphite, Liquid Phases, Solid Phases

Scientific paper

It is suggested in view of numerical calculations for white dwarf model atmospheres that, at optically transparent depths, layers of carbon can exist in the form of liquid droplets and graphite grains. The contribution of the condensate to the total opacity of the atmosphere will depend strongly on the model parameters, and may approach 100 percent.

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