Abstract
DQHerculis was the Summer 1997 WET northern hemisphere primary target. The O-C phase diagram of the 71s signal reveals out-of-eclipse phase variations resulting from the self eclipses of a nearly edge-on, non-axisymmetric disc. We investigate the problem of simulating DQ Herculis numerically, using the method of smoothed particle hydrodynamics (SPH), and from the time-averaged structure calculate the O-C phase variations as a function of inclination angle. The WET and SPH O-C phase variations match to a remarkable degree, and suggest a system inclination in the range 89.5° ≤ i ≤ 89.7°.
Original language | English |
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Pages (from-to) | 211-222 |
Number of pages | 12 |
Journal | Baltic Astronomy |
Volume | 9 |
Issue number | 2 |
DOIs | |
State | Published - 2000 |
Keywords
- Cataclysmic variables
- Individual: DQ Her
- Stars: binaries