X-ray Observation of SWIFT J1753.5-0127 with RXTE & XMM-Newton

Details X-ray Observation of SWIFT J1753.5-0127 with RXTE & XMM-Newton X-ray Observation of SWIFT J1753.5-0127 with RXTE & XMM-Newton

Oct 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1053..215s&link_type=abstract

OBSERVATIONAL EVIDENCE FOR BLACK HOLES IN THE UNIVERSE: Proceedings of the 2nd Kolkata Conference on Observational Evidence for

Computer Science

X-Ray Binaries, Galactic Nuclei, Circumnuclear Matter, And Bulges, X-Ray Emission Spectra And Fluorescence

Scientific paper

The X-ray transient source SWIFT J1753.5-0127 was identified to be a galactic black hole from the results of the analysis of RXTE and XMM-Newton data. We re-analyze the entire observational data made by RXTE and XMM-Newton to quantify the nature of X-ray emission by studying the accreting disk structure. Detailed timing and spectral studies support that the accretion disk was receding away from the compact object as indicated by the diminishing value of the QPO frequency from its highest value ~0.89 Hz to the minimum frequency (detectable). At the same time, the X-ray source remained in the low/hard state tending to go to harder state.

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