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Modelling two dust features in comet Hale-Bopp (1995 O1)

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dc.contributor.author Sekaniana, Z. en_US
dc.date.accessioned 2004-09-26
dc.date.available 2004-09-26
dc.date.issued 1997-03-20 en_US
dc.identifier.citation USA en_US
dc.identifier.clearanceno 97-0798 en_US
dc.identifier.uri http://hdl.handle.net/2014/22322
dc.description.abstract A Monte Carlo computer simulation code for generating synthetic images of dust features in comets is applied to comet Hale-Bopp to model the diurnal evolution of a bright jet and the appearance of nearly concentric halos. en_US
dc.format.extent 574519 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other comet-Hale-Bopp diurnal evolution of a dust jet dust halos nuclear rotation emission sources en_US
dc.title Modelling two dust features in comet Hale-Bopp (1995 O1) en_US


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