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dc.contributor.authorMurakawa, K.
dc.contributor.authorTamura, M.
dc.contributor.authorSuto, H.
dc.contributor.authorMiyata, T.
dc.contributor.authorGledhill, T.
dc.contributor.authorHough, J.
dc.date.accessioned2010-02-18T09:40:31Z
dc.date.available2010-02-18T09:40:31Z
dc.date.issued2003
dc.identifier.citationMurakawa , K , Tamura , M , Suto , H , Miyata , T , Gledhill , T & Hough , J 2003 , ' Near-infrared high imaging polarimetry of the Red Rectangle ' , Proceedings of the SPIE: Polarimetry in Astronomy , vol. 4843 , pp. 196-199 . https://doi.org/10.1117/12.458840
dc.identifier.otherPURE: 156828
dc.identifier.otherPURE UUID: 06fb356f-0b71-424d-aa1c-244900deb3ae
dc.identifier.otherdspace: 2299/4285
dc.identifier.otherScopus: 0038077569
dc.identifier.otherORCID: /0000-0002-2859-4600/work/30779780
dc.identifier.urihttp://hdl.handle.net/2299/4285
dc.descriptionCopyright 2003 Society of Photo-Optical Instrumentation Engineers. DOI: 10.1117/12.458840 [Full text of this paper is not available in the UHRA]
dc.description.abstractWe have carried out KHL band high resolution imaging and H band imaging-polarimetry of the Red Rectangle nebula using CIAO and 36 element AO mounted on the 8.2m Subaru telescope. HK band images show a X-shape structure close to 0.1 inch and 2 lobes with separation of 0.15 inch at the north and the south. Our L band image show a small clump and its position is 0.1 arcsec east from the center of the southern lobe. The polarization map shows roughly centrosymmetric vector pattern and the center of the pattern is consistent with that of 2 lobes. There is scatter of the vector pattern at approximately 0.1 inch east from the southern lobe and a local minimum in the degree of polarization. These results can explain that the primary star HD44179 is at 0.1 inch east from the southern lobes and the dominant illumination source is a M type star at the center of the nebula.en
dc.language.isoeng
dc.relation.ispartofProceedings of the SPIE: Polarimetry in Astronomy
dc.titleNear-infrared high imaging polarimetry of the Red Rectangleen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1117/12.458840
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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