Wet observations and smoothed particle simulations of DQ Herculis

M. A. Wood*, J. C. Simpson, S. D. Kawaler, M. S. O'Brien, R. E. Nather, T. S. Metcalfe, D. E. Winget, M. Montgomery, X. J. Jiang, E. M. Leibowitz, P. Ibbetson, D. O'Donoghue, J. Krzesinski, G. Pajdosz, S. Zola, G. Vauclair, N. Dolez, M. Chevreton

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

3 Scopus citations

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 languageEnglish
Pages (from-to)211-222
Number of pages12
JournalBaltic Astronomy
Volume9
Issue number2
DOIs
StatePublished - 2000

Keywords

  • Cataclysmic variables
  • Individual: DQ Her
  • Stars: binaries

Fingerprint

Dive into the research topics of 'Wet observations and smoothed particle simulations of DQ Herculis'. Together they form a unique fingerprint.

Cite this