A transient high-coherence oscillation in 4U 1820-30
Abstract
We re-analyzed two Rossi X-Ray Timing Explorer archival observations of the atoll source 4U 1820-30 in order to investigate the detailed time-frequency properties of the source during the intervals when a ~7 Hz QPO was detected by Wijnands et al. (1999, ApJ, 512, L39). We find that in both observations, in addition to a QPO signal lasting a couple of minutes as previously reported, there is a much narrower transient oscillation with a life time of only a few seconds. Within this time, the oscillation is consistent with being coherent. Its integrated fractional rms is around 10% and its frequency 7.3 Hz and 5.7 Hz in the two observations. We discuss the possible association of this QPO with other oscillations known both in Neutron-Star and Black-Hole systems, concentrating on the similarities with the narrow 5-7 Hz oscillations observed at high flux in Black-Hole Candidates.
Keywords
Cite
@article{arxiv.astro-ph/0405325,
title = {A transient high-coherence oscillation in 4U 1820-30},
author = {T. Belloni and I. Parolin and P. Casella},
journal= {arXiv preprint arXiv:astro-ph/0405325},
year = {2009}
}
Comments
5 pages, 3 figures, accepted for publication in A&A. FIgure 1 is reduced in resolution, full-resolution version of this text available at http://www.merate.mi.astro.it/~belloni/ms0335.ps.gz