Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/6851
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dc.contributor.authorJyothy, S. N-
dc.contributor.authorMurthy, J-
dc.contributor.authorKaruppath, N-
dc.contributor.authorSujatha, N. V-
dc.date.accessioned2015-10-19T11:55:14Z-
dc.date.available2015-10-19T11:55:14Z-
dc.date.issued2015-12-01-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, Vol. 454, No. 2, pp. 1778-1784en_US
dc.identifier.issn1365-2966-
dc.identifier.urihttp://hdl.handle.net/2248/6851-
dc.descriptionRestricted Accessen_US
dc.description.abstractWe present an analysis of the diffuse ultraviolet (UV) background in a low latitude region near the Aquila Rift based on observations made by the Galaxy Evolution Explorer (GALEX). The UV background is at a level of about 2000 ph cm−2 s−1 sr−1 Å−1 with no correlation with either the Galactic latitude or the 100 μm infrared (IR) emission. Rather, the UV emission falls off with distance from the bright B2 star HIP 88149, which is in the centre of the field. We have used a Monte Carlo model to derive an albedo of 0.6–0.7 in the UV with a phase function asymmetry factor (g) of 0.2–0.4. The value for the albedo is dependent on the dust distribution while g is determined by the extent of the halo.en_US
dc.language.isoenen_US
dc.publisherOxford University Press on behalf of the Royal Astronomical Societyen_US
dc.relation.urihttp://dx.doi.org/10.1093/mnras/stv2037-
dc.rights© Royal Astronomical Society-
dc.subjectDiffuse radiationen_US
dc.subjectUltraviolet: ISMen_US
dc.titleDiffuse radiation from the Aquila Riften_US
dc.typeArticleen_US
Appears in Collections:IIAP Publications

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