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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3620
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dc.contributor.authorShalima, P-
dc.contributor.authorMurthy, J-
dc.date.accessioned2008-09-15T14:31:24Z-
dc.date.available2008-09-15T14:31:24Z-
dc.date.issued2004-08-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 352, No. 4, pp. 1319 - 1322en
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2248/3620-
dc.description.abstractMurthy, Henry & Holberg discovered intense far-ultraviolet (FUV) (λλ912-1600) emission from the direction of the Coalsack molecular cloud 10 years ago. We have used their results in conjunction with a Monte Carlo model for the scattering in the region to show that the scattering is from dust in the foreground of the Coalsack. The albedo of the grains is 0.4 +/- 0.2. This is one of the few determinations of the albedo of dust in the diffuse interstellar medium in the FUV.en
dc.language.isoenen
dc.publisherRoyal Astronomical Societyen
dc.relation.urihttp://dx.doi.org/10.1111/j.1365-2966.2004.08022.xen
dc.subjectDusten
dc.subjectExtinctionen
dc.subjectUltraviolet: ISMen
dc.titleModelling of dust scattering toward the Coalsacken
dc.typeArticleen
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