AbstractUsing data from the All Sky Monitor (ASM) on the Rossi X-ray Timing Explorer (RXTE), we have searched for long term periodicities in the X-ray flux of GX 1+4, Sco X-2 (GX 349+2), and GX 339−4. For GX 1+4, we also used data from BATSE and Galactic Centre scans performed by RXTE. We find no evidence for X-ray modulations at the suggested ∼304d orbital period of GX 1+4. However, we find tentative evidence for a periodicity at 420–460d. An upper limit of 15% peak-to-peak is set on any sinusoidal modulation in the 1.5–3.0keV flux of Sco X-2 for periods in the 30–100d range. For GX 339−4, we confirm the Low State modulation and report the detection of significant low-frequency modulations in both the High State and Very High State. We fail to detect this modulation in the Off State. We show that if the reported orbital period of GX 339−4 lies in the range 0.5–1.7d, then it is not present in the RXTE ASM light curve.
Long-term periodicities in the flux from low mass X-ray binaries
Advances in Space Research ; 35 , 6 ; 1185-1191
2005-03-16
7 pages
Article (Journal)
Electronic Resource
English
Long-term periodicities in the flux from low mass X-ray binaries
British Library Conference Proceedings | 2005
|Long-term periodicities in the flux from low mass X-ray binaries
Online Contents | 2005
|On mid-term periodicities of high-latitude solar activity
Elsevier | 2014
|On mid-term periodicities of high-latitude solar activity
Online Contents | 2014
|