Simultaneous X-ray and Optical Observations of EX Hydrae
arXiv:astro-ph/0501087 · doi:10.1086/428487
Abstract
The intermediate polar, EX Hydrae, was the object of a large simultaneous multiwavelength observational campaign during 2000 May - June. Here we present the Rossi X-ray Timing Explorer photometry and optical photometry and spectroscopy from ground-based observatories obtained as part of this campaign. Balmer line radial velocities and Doppler maps provide evidence for an extended bulge along the outer edge of the accretion disk and some form of extended/overflowing material originating from the hot spot. In addition, the optical binary eclipse possesses an extended egress shoulder, an indication that an additional source (other than the white dwarf) is coming out of eclipse. We also compare the X-ray and optical results with the results obtained from the EUV and UV observations from the multiwavelength data set.
to appear in the Astronomical Journal, April 2005
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- New X-ray observations of the old nova CP Puppis and of the more recent nova V351 Pup
- Accretion column structure of magnetic cataclysmic variables from X-ray spectroscopy
- Steps towards a solution of the FS Aurigae puzzle. II. Confirmation of the intermediate polar status
- Peculiarities of the Accretion Flow in the System HL CMa
- Disc-Magnetosphere interactions in Cataclysmic Variable Stars