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Dust scattering from the taurus molecular cloud

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dc.contributor.author Sathya Narayan
dc.contributor.author Murthy, J
dc.contributor.author Narayanankutty, K
dc.date.accessioned 2020-11-17T14:11:29Z
dc.date.available 2020-11-17T14:11:29Z
dc.date.issued 2017-04
dc.identifier.citation Monthly Notices of the Royal Astronomical Society, Vol. 466, No. 3, pp. 3199-3205 en_US
dc.identifier.issn 1365-2966
dc.identifier.uri http://prints.iiap.res.in/handle/2248/7124
dc.description Restricted Access © Royal Astronomical Society https://doi.org/10.1093/mnras/stw3280 en_US
dc.description.abstract We present an analysis of the diffuse ultraviolet emission near the Taurus Molecular Cloud based on observations made by the Galaxy Evolution Explorer. We used a Monte Carlo dust scattering model to show that about half of the scattered flux originates in the molecular cloud with 25 per cent arising in the foreground and 25 per cent behind the cloud. The best-fitting albedo of the dust grains is 0.3, but the geometry is such that we could not constrain the phase function asymmetry factor (g). en_US
dc.language.iso en en_US
dc.publisher Oxford University Press on behalf of the Royal Astronomical Society en_US
dc.subject Ultraviolet: ISM en_US
dc.title Dust scattering from the taurus molecular cloud en_US
dc.type Article en_US


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