SIMBAD references

2003MNRAS.345L..35M - Mon. Not. R. Astron. Soc., 345, L35-L39 (2003/November-1)

Evidence of a decrease of kHz quasi-periodic oscillation peak separation towards low frequencies in 4U 1728-34 (GX 354-0).

MIGLIARI S., VAN DER KLIS M. and FENDER R.P.

Abstract (from CDS):

We have produced the colour-colour diagram of all the observations of 4U 1728-34 available in the Rossi X-ray Timing Explorer public archive (from 1996 to 2002) and found observations filling in a previously reported `gap' between the island and the banana X-ray states. We have made timing analysis of these gap observations and found, in one observation, two simultaneous kHz quasi-periodic oscillations (QPOs). The timing parameters of these kHz QPOs fit in the overall trend of the source. The `lower' kHz QPO has a centroid frequency of ∼308 Hz. This is the lowest `lower' kHz QPO frequency ever observed in 4U 1728-34. The peak frequency separation between the `upper' and the `lower' kHz QPO is Δν 274±11 Hz, significantly smaller than the constant value of Δν∼ 350 Hz found when the `lower' kHz QPO frequency is between ∼500 and 800 Hz. This is the first indication in this source for a significant decrease of kHz QPO peak separation towards low frequencies. We compare the result briefly to theoretical models for kHz QPO production.

Abstract Copyright: 2003 RAS

Journal keyword(s): accretion, accretion discs - binaries: close - stars: individual: 4U 1728 - stars: neutron

Simbad objects: 3

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