Morpho-Kinematical Modelling of Nova Eridani 2009 (KT Eri)

V A R M Ribeiro,Michael F Bode,M J Darnley,R Barnsley,Ulisse Munari,D J Harman

Monthly Notices of the Royal Astronomical Society（2013）

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摘要

Modelling the morphology of a nova outburst provides valuable information on the shaping mechanism in operation at early stages following the outburst. We performed morpho-kinematical studies, using SHAPE, of the evolution of the Hα line profile following the outburst of the nova KT Eridani. We applied a series of geometries in order to determine the morphology of the system. The best-fitting morp...

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关键词

line: profiles,stars: individual: KT Eridani,novae, cataclysmic variables

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