The XMM-Newton Slew view of IGRJ17361-4441: a transient in the globular cluster NGC 6388
arXiv:1203.0965 · doi:10.1016/j.newast.2012.02.001
Abstract
IGRJ17361-4441 is a hard transient recently observed by the INTEGRAL satellite. The source, close to the center of gravity of the globular cluster NGC 6388, quickly became the target of follow-up observations conducted by the Chandra, Swift/XRT and RXTE observatories. Here, we concentrate in particular on a set of observations conducted by the XMM-Newton satellite during two slews, in order to get the spectral information of the source and search for spectral variations. The spectral parameters determined by the recent XMM-Newton slew observations were compared to the previously known results. The maximum unabsorbed -ray flux in the 0.5-10 keV band as detected by the XMM-Newton slew observations is erg cm s, i.e. consistent with that observed by the Swift/XRT satellite 15 days earlier. The spectrum seems to be marginally consistent () with that derived from the previous high energy observation.
Accepted for publication on New Astronomy, 2012. A sentence about the globular cluster 47 Tuc was partially rewritten to avoid confusion
References in corpus (7)
- The first XMM-Newton slew survey catalogue: XMMSL1
- Refining the fundamental plane of accreting black holes
- The surface density profile of NGC 6388: a good candidate for harboring an intermediate-mass black hole
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Cited by in corpus (6)
- INTEGRAL/IBIS nine-year Galactic Hard X-Ray Survey
- INTEGRAL/IBIS 17-yr hard X-ray all-sky survey
- The puzzling source IGR J17361-4441 in NGC 6388: a possible planetary tidal disruption event
- X-ray Binaries in the Ultrahigh Encounter Rate Globular Cluster NGC 6388
- An XMM-Newton search for X-ray sources in the Fornax dwarf galaxy
- Searching for Intermediate Mass Black Holes in the Milky Way's galactic halo