| dc.contributor.author | Bailey, J. | |
| dc.contributor.author | Wickramasinghe, D.T. | |
| dc.contributor.author | Hough, J. | |
| dc.contributor.author | Cropper, M. | |
| dc.date.accessioned | 2009-04-17T14:08:02Z | |
| dc.date.available | 2009-04-17T14:08:02Z | |
| dc.date.issued | 1988 | |
| dc.identifier.citation | Bailey , J , Wickramasinghe , D T , Hough , J & Cropper , M 1988 , ' EXO 023432-5232.3 - an eclipsing AM Herculis binary ' , Monthly Notices of the Royal Astronomical Society , vol. 234 , no. 1 . | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.other | PURE: 152886 | |
| dc.identifier.other | PURE UUID: dd4400e6-04f4-4088-9da7-25abce3fabd4 | |
| dc.identifier.other | dspace: 2299/3202 | |
| dc.identifier.uri | http://hdl.handle.net/2299/3202 | |
| dc.description | Copyright Royal Astronomical Society. [Full text of this article is not available in the UHRA] | |
| dc.description.abstract | The authors report observations of the serendipitous EXOSAT source EXO 023432-5232.3 which confirm that the object is an AM Herculis type binary and show the presence of eclipses by the companion star. From high-speed photometry of the eclipses they deduce that the cyclotron emission region is less than one seventh the size of the white dwarf. From the infrared magnitude of the secondary a distance of 430 pc is deduced. The authors discuss constraints on the system geometry. | en |
| dc.language.iso | eng | |
| dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
| dc.title | EXO 023432-5232.3 - an eclipsing AM Herculis binary | 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 | |
