| dc.contributor.author | Peacock, T. | |
| dc.contributor.author | Cropper, M. | |
| dc.contributor.author | Bailey, J. | |
| dc.contributor.author | Hough, J. | |
| dc.contributor.author | Wickramasinghe, D.T. | |
| dc.date.accessioned | 2009-04-17T13:28:18Z | |
| dc.date.available | 2009-04-17T13:28:18Z | |
| dc.date.issued | 1992 | |
| dc.identifier.citation | Peacock , T , Cropper , M , Bailey , J , Hough , J & Wickramasinghe , D T 1992 , ' Polarimetry of ST LMi - Discovery of a second accreting pole ' , Monthly Notices of the Royal Astronomical Society , vol. 259 , no. 3 , pp. 583-592 . | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.other | PURE: 153357 | |
| dc.identifier.other | PURE UUID: 1178b440-f684-48ff-9cb0-459be9b94185 | |
| dc.identifier.other | dspace: 2299/3195 | |
| dc.identifier.uri | http://hdl.handle.net/2299/3195 | |
| dc.description | Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA] | |
| dc.description.abstract | We have obtained simultaneous multiband photometric and polarimetric light curves for ST LMi (CW1103 + 254) in the visible range and the near-infrared on three occasions. These clearly show the presence of previously unobserved accretion at or near the second magnetic pole of the white dwarf. The secondary accretion region is seen only in the H and J bands, from which we infer a lower accretion rate than for the primary region. | en |
| dc.language.iso | eng | |
| dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
| dc.title | Polarimetry of ST LMi - Discovery of a second accreting pole | en |
| dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
| dc.contributor.institution | Centre for Astrophysics Research | |
| dc.description.status | Peer reviewed | |
| rioxxterms.type | Journal Article/Review | |
| herts.preservation.rarelyaccessed | true | |
