Probing the nature of IGR J16493-4348: Spectral and temporal analysis of the 1-100 keV emission

Abstract

IGR J16493-4348 was one of the first new sources to be detected by the INTEGRAL gamma-ray telescope in the 18-100 keV energy band. Based upon spatial coincidence the source was originally associated with the free radio pulsar PSR J1649-4349. Presented here are the results of 2.8 Ms of observations made by the INTEGRAL mission and a 5.6 ks observation with the Swift X-ray Telescope. Spectral analysis indicates that the source is best modeled by an absorbed power law with a high energy cut-off at E${}_{cut}$~15 keV and a hydrogen absorbing column of NH=5.4${}_{-1}^{+1.3}$ x 10${}^{22}$ cm${}^{-2}$. Analysis of the light curves indicates that the source is a weak, persistent gamma-ray emitter showing indications of variability in the 2-9 and 22-100 keV bands. The average source flux is ~1.1 x 10^{-10} erg cm${}^{-2}$ s${}^{-1}$ in the 1-100 keV energy band. No coherent timing signal is identified at any timescale in the INTEGRAL or Swift data. The refined source location and positional uncertainty of IGR J16493-4348 places PSR J1649-4349 outside of the 90% error circle. We conclude that IGR J16493-4348 is not associated with PSR J1649-4349. Combining the INTEGRAL observations with Swift/XRT data and information gathered by RXTE and Chandra we suggest that IGR J16493-4348 is an X-ray binary; and that the source characteristics favour a high mass X-ray binary although an LMXB nature cannot be ruled out.

arXiv commentAccepted for publication in MNRAS. 7 pages, 5 figures (Note the resolution of figure 5 has been reduced)

References in corpus (13)

• The Leiden/Argentine/Bonn (LAB) Survey of Galactic HI: Final data release of the combined LDS and IAR surveys with improved stray-radiation corrections
• The Evolution and Structure of Pulsar Wind Nebulae
• The Parkes Multibeam Pulsar Survey: I. Observing and Data Analysis Systems, Discovery and Timing of 100 Pulsars
• The 3rd IBIS/ISGRI soft gamma-ray survey catalog
• The optical/NIR counterpart of the INTEGRAL obscured source IGR J16318-4848 : a sgB[e] in a HMXB ?
• The INTEGRAL IBIS/ISGRI System Point Spread Function and Source Location Accuracy
• A description of sources detected by INTEGRAL during the first 4 years of observations
• A refined position catalog of the Swift XRT afterglows
• The 1 - 50 keV spectral and timing analysis of IGR J18027-2016: an eclipsing, high mass X-ray binary
• BeppoSAX observations of the accretion-powered X-ray pulsar SMC X-1
• Global characteristics of the first IBIS/ISGRI catalogue sources: unveiling a murky episode of binary star evolution
• Unveiling the Nature of the High Energy Source IGR J19140+0951
• INTEGRAL observations of AGN obscured by the Galactic Plane

Cited by in corpus (8)

• Advances in Understanding High-Mass X-ray Binaries with INTEGRAL and Future Directions
• Superorbital Periodic Modulation in Wind-Accretion High-Mass X-ray Binaries from Swift BAT Observations
• The Swift-BAT hard X-ray sky monitoring unveils the orbital period of the HMXB IGR J16493-4348
• Evidence for a resonant cyclotron line in IGR J16493-4348 from the Swift-BAT hard X-ray survey
• Unveiling the nature of IGR J16493-4348 with IR spectroscopy
• A Study of the 20 Day Superorbital Modulation in the High-Mass X-ray Binary IGR J16493-4348
• The Orbital Parameters of the Eclipsing High-Mass X-ray Binary Pulsar IGR J16493-4348 from Pulsar Timing
• Comprehensive broadband study of accreting neutron stars with Suzaku: Is there a bi-modality in the X-ray spectrum?