AN ULTRA-FAST X-RAY DISK WIND IN THE NEUTRON STAR BINARY GX 340+0

We present a spectral analysis of a brief Chandra/HETG observation of the neutron star low-mass X-ray binary GX 340+0. The high-resolution spectrum reveals evidence of ionized absorption in the Fe K band. The strongest feature, an absorption line at approximately 6.9 keV, is required at the 5σ level...

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Bibliographic Details
Main Authors: Miller, J. M. (Author), Raymond, J. (Author), Cackett, E. (Author), Grinberg, Victoria (Contributor), Nowak, Michael A. (Author)
Other Authors: MIT Kavli Institute for Astrophysics and Space Research (Contributor), Nowak, Michael A (Contributor)
Format: Article
Language:English
Published: IOP Publishing, 2017-07-12T18:06:44Z.
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