Suzaku observation of IGR J16318-4848

Barragan L, Wilms J, Pottschmidt K, Nowak MA, Kreykenbohm I, Walter R, Tomsick JA (2009)


Publication Status: Published

Publication Type: Journal article

Publication year: 2009

Journal

Publisher: EDP SCIENCES S A

Book Volume: 508

Pages Range: 1275-1278

Journal Issue: 3

DOI: 10.1051/0004-6361/200810811

Abstract

We report on the first Suzaku observation of IGR J16318-4848, the most extreme example of a new group of highly absorbed X-ray binaries that have recently been discovered by the International Gamma-Ray Astrophysics Laboratory (INTEGRAL). The Suzaku observation was carried out between 2006 August 14 and 17, with a net exposure time of 97 ks.The average X-ray spectrum of the source can be well described (chi(2)(red) = 0.99) with a continuum model typical for neutron stars i.e., a strongly absorbed power law continuum with a photon index of 0.676(42) and an exponential cutoff at 20.5(6) keV. The absorbing column is N-H = 1.95(3) x 10(24) cm(-2). Consistent with earlier work, strong fluorescent emission lines of Fe K alpha, Fe K beta, and Ni K alpha are observed. Despite the large N-H, no Compton shoulder is seen in the lines, arguing for a non-spherical and inhomogeneous absorber. Seen at an average 5-60 keV absorbed flux of 3.4x10(-10) erg cm(-2) s(-1), the source exhibits significant variability on timescales of hours.

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APA:

Barragan, L., Wilms, J., Pottschmidt, K., Nowak, M.A., Kreykenbohm, I., Walter, R., & Tomsick, J.A. (2009). Suzaku observation of IGR J16318-4848. Astronomy & Astrophysics, 508(3), 1275-1278. https://dx.doi.org/10.1051/0004-6361/200810811

MLA:

Barragan, L., et al. "Suzaku observation of IGR J16318-4848." Astronomy & Astrophysics 508.3 (2009): 1275-1278.

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