The Power Spectral Properties of the Z Source Gx 340+0

We present an analysis of ∼390 ksec of data of the Z source GX 340+0 taken during 24 observations with the Rossi X -rayTiming Explorer satellite. We report the discovery of a new broad component in the power spectra. The frequency of this component varied between 9 and 14 Hz, and remained close to half that of the horizontal branch quasi-periodic oscillations (HBO). Its rms amplitude was consistent with being constant around ∼5%, while its FWHM increased with frequency from 7 to 18 Hz. If this sub-HBO component is the fundamental frequency, then the HBO and its second harmonic are the second and fourth harmonic component, while the third harmonic was not detected. This is similar to what was recently found for the black hole candidate XTE J1550–564. The profiles of both the horizontaland the normal branch quasi-periodic oscillation peaks were asymmetric when they were strongest. We describe this in terms of a shoulder component at the high frequency side of the quasi-periodic oscillation peak, whose rms amplitudes were approximately constant at ∼4% and ∼3%, respectively. The peak separation between the twin kHz quasi-periodic oscillations was consistent with being constant at 339±8 Hz but a trend similar to that seen in, e.g. Sco X–1 could not be excluded. We discuss our results within the framework of the various models which have been proposed for the kHz QPOs and low frequency peaks. Subject headings: accretion, accretion disks — stars: individual (GX340+0) — stars: neutron — X-rays: stars