Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3620
Title: Modelling of dust scattering toward the Coalsack
Authors: Shalima, P
Murthy, J
Keywords: Dust;Extinction;Ultraviolet: ISM
Issue Date: Aug-2004
Publisher: Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, Vol. 352, No. 4, pp. 1319 - 1322
Abstract: Murthy, 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.
URI: http://hdl.handle.net/2248/3620
ISSN: 0035-8711
???metadata.dc.relation.uri???: http://dx.doi.org/10.1111/j.1365-2966.2004.08022.x
Appears in Collections:IIAP Publications

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