English

Superhumps and their Evolution during Superoutbursts

Solar and Stellar Astrophysics 2016-05-10 v1

Abstract

Light curves of superhumps and their evolution during superoutbursts are analyzed by decomposing them into their Fourier components, including the fundamental mode and the first three overtones. The amplitudes of the fundamental mode are found to decrease significantly during superoutburst while those of the overtones remain practically constant. The phases of maxima of the fundamental mode {\it increase} systematically during superoutburst while those of the overtones -- systematically {\it decrease}. The combination of the two effects is responsible for the characteristic evolution of superhump light curves: the appearance and growth of the secondary humps and the spurious phase jumps in the (O-C) diagrams. Two intrepretations are possible. Either that instead of just one superhump period PshP_{sh} there are four periods PkP_k which resemble -- but are significantly different from -- the fundamental mode and the first three overtones of PshP_{sh}. Or -- more likely -- that those time-dependent phase shifts are genuine.

Cite

@article{arxiv.1602.06702,
  title  = {Superhumps and their Evolution during Superoutbursts},
  author = {J. Smak},
  journal= {arXiv preprint arXiv:1602.06702},
  year   = {2016}
}

Comments

9 pages, 4 figures; submitted to "Acta Astronomica"

R2 v1 2026-06-22T12:54:55.603Z