| dc.contributor.author | Bailey, J. | |
| dc.contributor.author | Hough, J. | |
| dc.contributor.author | Gilmozzi, R. | |
| dc.contributor.author | Axon, D.J. | |
| dc.date.accessioned | 2009-04-20T13:35:00Z | |
| dc.date.available | 2009-04-20T13:35:00Z | |
| dc.date.issued | 1984 | |
| dc.identifier.citation | Bailey , 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.issn | 0035-8711 | |
| dc.identifier.other | dspace: 2299/3225 | |
| dc.identifier.uri | http://hdl.handle.net/2299/3225 | |
| dc.description | Original 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.abstract | Circular 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.iso | eng | |
| dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
| dc.title | Infrared and optical polarimetry of AM Herculis | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
| dc.description.status | Peer reviewed | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
