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dc.contributor.authorBerriman, G.
dc.contributor.authorBailey, J.
dc.contributor.authorAxon, D.J.
dc.contributor.authorHough, J.
dc.date.accessioned2009-04-20T10:15:15Z
dc.date.available2009-04-20T10:15:15Z
dc.date.issued1986
dc.identifier.citationBerriman , G , Bailey , J , Axon , D J & Hough , J 1986 , ' The origin of the visual and infrared pulsations in the intermediate polar FO AQR (H2215-086) ' , Monthly Notices of the Royal Astronomical Society , vol. 223 , no. 3 , pp. 449-455 .
dc.identifier.issn0035-8711
dc.identifier.otherdspace: 2299/3211
dc.identifier.urihttp://hdl.handle.net/2299/3211
dc.descriptionOriginal article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractSimultaneous visual and infrared polarimetry of the intermediate polar FO Aqr (H2215-086) shows that its visual and infrared pulsations, seen at the rotation period of the white dwarf, are not circularly polarized. This is despite the fact that the infrared pulsations come from optically thin material: if cyclotron emission is important, it must be efficiently depolarized without the pulsations being hidden. The authors describe how this may come about, and discuss what further measurements will best establish whether cyclotron emission is important. The visual pulsations come from opaque material, and most likely arise from reprocessing at the surface of the white dwarf, but the possibility that cyclotron emission is important in the visual too cannot be definitely excluded.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleThe origin of the visual and infrared pulsations in the intermediate polar FO AQR (H2215-086)en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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