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- W2564402006 abstract "We present an analysis of the diffuse ultraviolet (UV) emission near the Taurus Molecular Cloud based on observations made by the Galaxy Evolution Explorer (GALEX). We used a Monte Carlo dust scattering model to show that about half of the scattered flux originates in the molecular cloud with 25% arising in the foreground and 25% behind the cloud. The best-fit albedo of the dust grains is 0.3 but the geometry is such that we could not constrain the phase function asymmetry factor (g)." @default.
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- W2564402006 date "2016-12-17" @default.
- W2564402006 modified "2023-10-16" @default.
- W2564402006 title "Dust scattering from the Taurus Molecular Cloud" @default.
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- W2564402006 doi "https://doi.org/10.1093/mnras/stw3280" @default.
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