Abstract
We report on a comprehensive analysis of simultaneous X-ray polarimetric and spectral data of the bright atoll source GX 9+9 with the Imaging X-ray Polarimetry Explorer (IXPE) and NuSTAR. The source is significantly polarized in the 4- 8 keV band, with a degree of 2.2% ± 0.5% (uncertainty at the 68% confidence level). The NuSTAR broad-band spectrum clearly shows an iron line, and is well described by a model including thermal disc emission, a Comptonized component, and reflection. From a spectro-polarimetric fit, we obtain an upper limit to the polarization degree of the disc of 4% (at the 99% confidence level), while the contribution of Comptonized and reflected radiation cannot be conclusively separated. However, the polarization is consistent with resulting from a combination of Comptonization in a boundary or spreading layer, plus reflection off the disc, which significantly contributes in any realistic scenario.
| Original language | English |
|---|---|
| Article number | A20 |
| Journal | Astronomy and Astrophysics |
| Volume | 676 |
| DOIs | |
| State | Published - Aug 1 2023 |
Keywords
- Accretion
- Accretion disks
- Polarization
- Stars: neutron
- X-rays: binaries
- X-rays: general
- X-rays: individuals: GX 9+9