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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6746
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dc.contributor.authorMuthumariappan, C-
dc.contributor.authorParthasarathy, M-
dc.contributor.authorIta, Y-
dc.date.accessioned2020-11-10T02:37:54Z-
dc.date.available2020-11-10T02:37:54Z-
dc.date.issued2015-08-
dc.identifier.citationASP conference series; Vol. 497, pp. 493- 494en_US
dc.identifier.isbn978-1-58381-878-7-
dc.identifier.urihttp://prints.iiap.res.in/handle/2248/6746-
dc.descriptionrestricted access © Astronomical Society of the Pacific http://aspbooks.org/custom/publications/paper/497-0493.htmlen_US
dc.description.abstractWe report results from our 1-D radiative transfer modelling of dust in the hydrogen-deficient planetary nebula IRAS 18333-2357 and discuss the properties of classical-grain and very small-grain populations of this PN.en_US
dc.language.isoenen_US
dc.publisherAstronomical Society of the Pacificen_US
dc.titleRadiative Transfer Modelling of Dust in the M22 PN IRAS 18333-2357en_US
dc.typeBooken_US
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