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dc.contributor.authorBailey, J.
dc.contributor.authorWickramasinghe, D.T.
dc.contributor.authorHough, J.
dc.contributor.authorCropper, M.
dc.date.accessioned2009-04-17T14:08:02Z
dc.date.available2009-04-17T14:08:02Z
dc.date.issued1988
dc.identifier.citationBailey , 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.issn0035-8711
dc.identifier.otherPURE: 152886
dc.identifier.otherPURE UUID: dd4400e6-04f4-4088-9da7-25abce3fabd4
dc.identifier.otherdspace: 2299/3202
dc.identifier.urihttp://hdl.handle.net/2299/3202
dc.descriptionCopyright Royal Astronomical Society. [Full text of this article is not available in the UHRA]
dc.description.abstractThe 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.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleEXO 023432-5232.3 - an eclipsing AM Herculis binaryen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1988
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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