An unusual Eddington-limited thermonuclear X-ray burst was detected from the accreting neutron star in 2S 0918-549 with the Rossi X-ray Timing Explorer. The burst commenced with a brief (40 ms) precursor and maintained near-Eddington fluxes during the initial 77 s. These characteristics are indicative of a nova-like expulsion of a shell from the neutron star surface. Starting 122 s into the burst, the burst shows strong (87 +/- 1% peak-to-peak amplitude) achromatic fluctuations for 60 s. We speculate that the fluctuations are due to Thompson scattering by fully-ionized inhomogeneities in a resettling accretion disk that was disrupted by the effects of super-Eddington fluxes. An expanding shell may be the necessary prerequisite for the fluctuations.
@article{arxiv.1009.5359,
title = {Achromatic late-time variability in thermonuclear X-ray bursts - an accretion disk disrupted by a nova-like shell?},
author = {J. J. M. in 't Zand and D. K. Galloway and D. R. Ballantyne},
journal= {arXiv preprint arXiv:1009.5359},
year = {2015}
}