The properties of the dust around Nova V705 Cas

Details The properties of the dust around Nova V705 Cas The properties of the dust around Nova V705 Cas

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..637..275e&link_type=abstract

CLASSICAL NOVA EXPLOSIONS: International Conference on Classical Nova Explosions. AIP Conference Proceedings, Volume 637, pp. 2

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Novae, Dwarf Novae, Recurrent Novae, And Other Cataclysmic Variables, Dust Processes

Scientific paper

Nova V705 Cas (1993) was an archetypical dust-forming nova. It displayed a deep minimum in the visual light curve, and spectroscopic evidence for carbon, hydrocarbon and silicate dust. We report preliminary results of work in progress, in which we use the DUSTY code to determine the properties of the dust. Our results have implications for the rate of grain growth in the ejecta, and for the origin of the UIR features; the latter likely arise in hydrogenated amorphous carbon grains rather than in free-flying PAH molecules.

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