Please use this identifier to cite or link to this item: https://doi.org/10.1007/BF00651869
DC FieldValue
dc.titleOn the moment method for radiative transfer in spherical dust shells with a core
dc.contributor.authorWilson, S.J.
dc.contributor.authorWan, F.S.
dc.contributor.authorSen, K.K.
dc.date.accessioned2014-10-28T02:41:48Z
dc.date.available2014-10-28T02:41:48Z
dc.date.issued1980-01
dc.identifier.citationWilson, S.J., Wan, F.S., Sen, K.K. (1980-01). On the moment method for radiative transfer in spherical dust shells with a core. Astrophysics and Space Science 67 (1) : 99-103. ScholarBank@NUS Repository. https://doi.org/10.1007/BF00651869
dc.identifier.issn0004640X
dc.identifier.urihttp://scholarbank.nus.edu.sg/handle/10635/103815
dc.description.abstractA two-shell moment method with three stream division of the radiation field has been suggested for solving radiative transfer problems in a non-grey extended dust shell surrounding a central star. The results computed are found to be of comparable accuracy with those of Unno and Kondo, obtained by generalized Eddington approximation. A more simplified approximation has been put forward for an optically thin medium. © 1980 D. Reidel Publishing Co.
dc.description.urihttp://libproxy1.nus.edu.sg/login?url=http://dx.doi.org/10.1007/BF00651869
dc.sourceScopus
dc.typeArticle
dc.contributor.departmentMATHEMATICS
dc.description.doi10.1007/BF00651869
dc.description.sourcetitleAstrophysics and Space Science
dc.description.volume67
dc.description.issue1
dc.description.page99-103
dc.identifier.isiutA1980JD39500006
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