Abstract
We present high-speed photometric observations of FS Aur taken with the 4.2m WHT and the high-speed camera ULTRACAM. These observations were intended to search for fluctuations on timescales 50-100 sec. We detected oscillations with a period of about 100 sec, seen repeatedly for a short time of every half of the orbital period. These oscillations support our hypothesis on the precession of the rapidly rotating white dwarf in FS Aur.
Original language | English (Ireland) |
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Title of host publication | Astrophysics of Cataclysmic Variables and Related Objects |
Publisher | ASTRONOMICAL SOC PACIFIC |
Number of pages | 1 |
Volume | 330 |
Publication status | Published - 1 Jan 2005 |
Authors (Note for portal: view the doc link for the full list of authors)
- Authors
- Neustroev, VV;Shearer, A;Zharikov, SV;Tovmassian, GH