Kilohertz QPOs, spectral state transitions and the distance to the neutron star X-ray transient IGR J17473-2721.

D. Altamirano*, D. Galloway, J. Chenevez, J. in´t Zand, E. Kuulkers, N. Degenaar, E. del Monte, M. Feroci, Y. Evangelista, M. Falanga, C. Markwardt, R. Wijnands, M. van der Klis

*Corresponding author for this work

    Research output: Other contributionNet publication - Internet publicationResearch


    We report on RXTE monitoring observations of the transient X-ray binary IGR J17473-2721 since the beginning of its latest outburst on March 26th, 2008 (see ATEL #1445, #1459, #1460, #1461 and #1468). IGR J17473-2721 reached a maximum unabsorbed flux of ~1.30E-8 ergs cm-2 s-1 (2-10 keV, assuming nH=3.8e22cm-2, ATEL #1459) on June 22nd, and has been steadily decreasing since. The X-ray spectral state (based on the X-ray colors in the 2-16 keV band) has switched from hard to soft and back to hard. These state changes are also evident from the Swift/BAT Hard X-ray monitoring light curves. During the soft state, 6 observations show a significant (between 3.5 and 10 sigma) kHz QPO at frequency up to ~900 Hz, that reach up to 8% rms amplitudes (2-60 keV). The combination of energy spectral and power spectral variations are typical of neutron star atoll sources. RXTE has detected 16 type-I (thermonuclear) X-ray bursts so far during this outburst. Two bursts observed on July 17 and 19 exhibited photospheric radius expansion, reaching identical peak (bolometric) fluxes of 9.5e-8 erg/cm2/s. The corresponding distance is likely between 4.9 kpc (using the theoretical Eddington limit for a pure He atmosphere) and 5.7 kpc (using the empirical value for the Eddington luminosity from Kuulkers et al. 2003, A&A, 399, 663). We found no evidence for burst oscillations.
    Original languageEnglish
    Publication date8 Aug 2008
    Publication statusPublished - 8 Aug 2008
    SeriesThe Astronomer's telegram
    NumberATel #1651


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