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dc.contributor.authorBailey, J.
dc.contributor.authorHough, J.
dc.contributor.authorGilmozzi, R.
dc.contributor.authorAxon, D.J.
dc.date.accessioned2009-04-20T13:35:00Z
dc.date.available2009-04-20T13:35:00Z
dc.date.issued1984
dc.identifier.citationBailey , J , Hough , J , Gilmozzi , R & Axon , D J 1984 , ' Infrared and optical polarimetry of AM Herculis ' , Monthly Notices of the Royal Astronomical Society , vol. 207 , no. 4 , pp. 777-782 .
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 153001
dc.identifier.otherPURE UUID: f0cb7498-5081-447f-8d35-3470ece02cb3
dc.identifier.otherdspace: 2299/3225
dc.identifier.urihttp://hdl.handle.net/2299/3225
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.abstractCircular polarization observations of AM Herculis have been obtained at wavelengths from 0.55 micron (V) to 2.2 micron (K) using a simultaneous three-channel polarimeter. Polarizations of up to 20 per cent were observed at 2.2 micron, as high as those observed at any other wavelength. The form of the polarization curve showed substantial wavelength dependence with the 2.2 micron polarization being limited to a feature lasting for around 30 per cent of the cycle. The observations are discussed in terms of cyclotron models.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleInfrared and optical polarimetry of AM Herculisen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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