WW horologii: X-ray and optical observations
| dc.contributor.author | Tennant, Allyn F. | en |
| dc.contributor.author | Bailey, Jeremy | en |
| dc.contributor.author | Wickramasinghe, D. T. | en |
| dc.contributor.author | Wu, Kinwah | en |
| dc.contributor.author | Ferrario, Lilia | en |
| dc.contributor.author | Hough, J. | en |
| dc.date.accessioned | 2026-01-01T15:42:23Z | |
| dc.date.available | 2026-01-01T15:42:23Z | |
| dc.date.issued | 1994 | en |
| dc.description.abstract | The eclipsing AM Herculis binary WW Hor (EXO 023432-5232.3) was observed in the X-ray band with the ROSAT satellite and in the optical band with the 3.9-m telescope of the Anglo-Australian Observatory. A clear eclipse is seen in the X-ray light curve of this system for the first time. The relative location of the X-ray eclipse suggests that the accretion pole on the white dwarf surface has migrated in the last few years, consistent with the optical data. The 0.2-2 keV spectrum is well fitted with an absorbed power-law model. There is no indication of a soft blackbody component, although such a component could be masked by the absorption. The X-ray luminosity of the system in the 0.2-2 keV band is 1.0 | en |
| dc.description.status | Peer-reviewed | en |
| dc.format.extent | 4 | en |
| dc.identifier.issn | 0035-8711 | en |
| dc.identifier.scopus | 0042365541 | en |
| dc.identifier.uri | https://hdl.handle.net/1885/733801440 | |
| dc.language.iso | en | en |
| dc.rights | Publisher Copyright: © Royal Astronomical Society. | en |
| dc.source | Monthly Notices of the Royal Astronomical Society | en |
| dc.subject | Binaries: close | en |
| dc.subject | Cataclysmic variables | en |
| dc.subject | Novae | en |
| dc.subject | Stars: individual: WW Hor | en |
| dc.subject | Stars: magnetic fields | en |
| dc.subject | X-rays: stars | en |
| dc.title | WW horologii: X-ray and optical observations | en |
| dc.type | Journal article | en |
| dspace.entity.type | Publication | en |
| local.bibliographicCitation.lastpage | 736 | en |
| local.bibliographicCitation.startpage | 733 | en |
| local.contributor.affiliation | Tennant, Allyn F.; NASA Marshall Space Flight Center | en |
| local.contributor.affiliation | Bailey, Jeremy; Australian Astronomical Observatory | en |
| local.contributor.affiliation | Wickramasinghe, D. T.; Mathematical Sciences Institute Research, Mathematical Sciences Institute, ANU College of Systems and Society, The Australian National University | en |
| local.contributor.affiliation | Wu, Kinwah; University of Sydney | en |
| local.contributor.affiliation | Ferrario, Lilia; Department of Mathematics | en |
| local.contributor.affiliation | Hough, J.; University of Hertfordshire | en |
| local.identifier.citationvolume | 271 | en |
| local.identifier.doi | 10.1093/mnras/271.3.733 | en |
| local.identifier.pure | a12f5cb5-bf24-4ebf-b5f6-5790471b3529 | en |
| local.identifier.url | https://www.scopus.com/pages/publications/0042365541 | en |
| local.type.status | Published | en |