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Paper detail

Swift, INTEGRAL, RXTE, and Spitzer reveal IGR J16283-4838

We present the first combined study of the recently discovered source IGR J16283-4838 with Swift, INTEGRAL, and RXTE. The source, discovered by INTEGRAL on April 7, 2005, shows a highly absorbed (variable N_H = 0.4 - 1.7 x 1e23 1/cm**2) and flat (photon index = 1) spectrum in the Swift/XRT and RXTE/PCA data. No optical counterpart is detectable (V > 20 mag), but a possible infrared counterpart within the Swift/XRT error radius is detected in the 2MASS and Spitzer/GLIMPSE survey. The observations suggest that IGR J16283-4838 is a high mass X-ray binary containing a neutron star embedded in Compton thick material. This makes IGR J16283-4838 a member of the class of highly absorbed HMXBs, discovered by INTEGRAL.

preprint2005arXivOpen access
V. BeckmannJ. A. KenneaC. MarkwardtA. PaizisS. SoldiJ. RodriguezS. D. BarthelmyD. N. BurrowsM. ChesterN. GehrelsN. MowlaviJ. Nousek
astro-ph
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V. BeckmannJ. A. KenneaC. MarkwardtA. PaizisS. SoldiJ. RodriguezS. D. BarthelmyD. N. BurrowsM. ChesterN. GehrelsN. MowlaviJ. Nousek

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