http://arxiv.org/abs/1906.08037
We report the first discovery of pulse phase modulating optical depths at the iron K-edge in accretion-powered X-ray pulsars, from Suzaku observations. A significant modulating optical depth of the iron K-edge is detected for Vela X-1 and GX 1+4. Similar trends are seen in GX 301-2 and OAO 1657-415, though with poor statistical significance. The observed iron K-edge exhibits a maximum optical depth, when the X-ray continuum dims, and there is no significant pulse phase variation in the ionization state of iron. The revealed changes in the optical depth with pulse phase can be explained as being due to the accreting matter captured by the magnetic field lines of the pulsar, which co-rotates with the neutron star spin and is responsible for photoelectric absorption. Based on the above interpretation, we propose that the accreting matter within the Alfv\’en radius contains iron with an ionization state of Fe$_{\rm V\hspace{-0.1em}I-X\hspace{-0.1em}I}$ with a particle density of $10^{17}$ cm$^{-3}$ and has a shape flattened along the azimuthal direction, such as an accretion curtain.
Y. Yoshida and S. Kitamoto
Thu, 20 Jun 19
10/51
Comments: 22pages, 13 figures, Accepted for publication in the Astrophysical Journal