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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1912
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dc.contributor.authorVaidya, D. B-
dc.contributor.authorAnandarao, B. G-
dc.contributor.authorDesai, J. N-
dc.date.accessioned2007-10-19T11:08:05Z-
dc.date.available2007-10-19T11:08:05Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 1, pp. 141 - 144en
dc.identifier.urihttp://hdl.handle.net/2248/1912-
dc.description.abstractUsing discrete dipole approximation (DDA) we calculate the extinction efficiencies of the porous silicate grains. We use these efficiencies to reproduce the observed extinction in the region of star formation in Orion and find that the grain models with about 40 percent porosity fit the observed extinction reasonably well.en
dc.format.extent198786 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..141Ven
dc.subjectInterstellaren
dc.subjectOrionen
dc.titleInterstellar grains towards Orionen
dc.typeArticleen
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