Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/7532
Title: Components of the diffuse ultraviolet radiation at high latitudes
Authors: Akshaya, M. S
Murthy, J
Ravichandran, S
Henry, R. C
Overduin, J
Keywords: ISM: Clouds;Dust;Extinction;Diffuse radiation;Ultraviolet;ISM
Issue Date: Oct-2019
Publisher: Oxford University Press on behalf of the Royal Astronomical Society
Citation: Monthly Notices of the Royal Astronomical Society, Vol. 489, No. 1, pp.1120–1126
Abstract: We have used data from the Galaxy Evolution Explorer to study the different components of the diffuse ultraviolet background in the region between the Galactic latitudes 70°–80°. We find an offset at zero dust column density (E(B − V) = 0) of 240 ± 18 photon units in the FUV (1539 Å) and 394 ± 37 photon units in the NUV (2316 Å). This is approximately half of the total observed radiation with the remainder divided between an extragalactic component of 114 ± 18 photon units in the FUV and 194 ± 37 photon units in the NUV and starlight scattered by Galactic dust at high latitudes. The optical constants of the dust grains were found to be a = 0.4 ± 0.1 and g = 0.8 ± 0.1 (FUV) and a = 0.4 ± 0.1 and g = 0.5 ± 0.1 (NUV). We cannot differentiate between a Galactic or extragalactic origin for the zero-offset but can affirm that it is not from any known source.
Description: Restricted Access
URI: http://hdl.handle.net/2248/7532
ISSN: 1365-2966
???metadata.dc.rights???: © Royal Astronomical Society
???metadata.dc.relation.uri???: https://doi.org/10.1093/mnras/stz2186
Appears in Collections:IIAP Publications

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