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) |
|---|---|
| Title of host publication | Astrophysics of Cataclysmic Variables and Related Objects |
| Publication status | Published - 1 May 2005 |
Authors (Note for portal: view the doc link for the full list of authors)
- Authors
- Neustroev, VV,Shearer, A,Zharikov, SV,Tovmassian, GH,Hameury, JM,Lasota, JP