Possible role of the white dwarf in grain formation in cataclysmic variable systems

Details Possible role of the white dwarf in grain formation in cataclysmic variable systems Possible role of the white dwarf in grain formation in cataclysmic variable systems

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.131..443a&link_type=abstract

(IAU, Colloquium on Cataclysmic Variables. Recent Multi-Frequency Observations and Theoretical Developments, 93rd, Bamberg, West

Astronomy and Astrophysics

Astrophysics

4

Cataclysmic Variables, Crystallization, Grain Size, Radiation Pressure, Stellar Mass Ejection, White Dwarf Stars, Carbon, Cosmic Dust, Phase Diagrams, Stellar Atmospheres, Stellar Envelopes

Scientific paper

The authors consider the possibility that carbon, in the form of the
allotrope carbyne, might form in the atmosphere of the white dwarf in a
cataclysmic variable system, and be expelled from the system by
radiation pressure. It seems that, under some circumstances, cataclysmic
variable systems may indeed have carbon dust in their vicinity.

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