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dc.contributor.authorBailey, J.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorHough, J.
dc.contributor.authorGledhill, T.
dc.contributor.authorMcCall, A.
dc.contributor.authorClark, S.
dc.contributor.authorMenard, F.
dc.contributor.authorTamura, M.
dc.date.accessioned2008-11-27T09:23:09Z
dc.date.available2008-11-27T09:23:09Z
dc.date.issued1998
dc.identifier.citationBailey , J , Chrysostomou , A , Hough , J , Gledhill , T , McCall , A , Clark , S , Menard , F & Tamura , M 1998 , ' Circular Polarization in Star- Formation Regions : Implications for Biomolecular Homochirality ' , Science , vol. 281 , no. 5377 , pp. 672-674 . https://doi.org/10.1126/science.281.5377.672
dc.identifier.issn0036-8075
dc.identifier.otherPURE: 151189
dc.identifier.otherPURE UUID: fafa3e0f-e1d6-4b92-ad09-0c8b796680fa
dc.identifier.otherdspace: 2299/2653
dc.identifier.otherScopus: 0032584646
dc.identifier.otherORCID: /0000-0002-2859-4600/work/30779799
dc.identifier.urihttp://hdl.handle.net/2299/2653
dc.descriptionOriginal article can be found at: http://www.sciencemag.org/magazine.dtl Copyright AAAS DOI: 10.1126/science.281.5377.672 [Full text of this article is not available in the UHRA]
dc.description.abstractStrong infrared circular polarization resulting from dust scattering in reflection nebulae in the Orion OMC-1 star-formation region has been observed. Circular polarization at shorter wavelengths might have been important in inducing chiral asymmetry in interstellar organic molecules that could be subsequently delivered to the early Earth by comets, interplanetary dust particles, or meteors. This could account for the excess of l–amino acids found in the Murchison meteorite and could explain the origin of the homochirality of biological molecules.en
dc.language.isoeng
dc.relation.ispartofScience
dc.titleCircular Polarization in Star- Formation Regions : Implications for Biomolecular Homochiralityen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1126/science.281.5377.672
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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