Dust in Nova Systems - Thoughts in Transition

Details Dust in Nova Systems - Thoughts in Transition Dust in Nova Systems - Thoughts in Transition

Jun 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983qjras..24...83b&link_type=abstract

Quarterly Journal of the Royal Astronomical Society, Vol. 24, P. 83, 1983

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18

Scientific paper

The authors review the evidence for the presence of dust around cataclysmic variables, with particular emphasis on classical novae. Two general models - rapid grain formation and pre-existing grains - for the infrared development of novae are critically discussed and relevant observations of other cataclysmic variables that have some bearing on these models are described.

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