1. First spectropolarimetric observation of the neutron star low-mass X-ray binary GX 3+1
- Author
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Gnarini, Andrea, Farinelli, Ruben, Ursini, Francesco, Bianchi, Stefano, Capitanio, Fiamma, Matt, Giorgio, Ng, Mason, Tarana, Antonella, Bobrikova, Anna, Cocchi, Massimo, Fabiani, Sergio, Kaaret, Philip, Poutanen, Juri, and Ravi, Swati
- Subjects
Astrophysics - High Energy Astrophysical Phenomena - Abstract
We report the first simultaneous X-ray spectropolarimetric observation of the bright atoll neutron star low-mass X-ray binary GX 3+1, performed by the Imaging X-ray Polarimetry Explorer (IXPE) joint with NICER and NuSTAR. The source does not exhibit significant polarization in the 2-8 keV energy band, with an upper limit of 1.3% at a 99% confidence level on the polarization degree. The observed spectra can be well described by a combination of thermal disk emission, the hard Comptonization component, and reflected photons off the accretion disk. In particular, from the broad Fe K$\alpha$ line profile, we were able to determine the inclination of the system ($i \approx 36^\circ$), which is crucial for comparing the observed polarization with theoretical models. Both the spectral and polarization properties of GX 3+1 are consistent with those of other atoll sources observed by IXPE. Therefore, we may expect a similar geometrical configuration for the accreting system and the hot Comptonizing region. The low polarization is also consistent with the low inclination of the system., Comment: 7 pages, 6 figures, 4 tables. Accepted for publication in Astronomy & Astrophysics. arXiv admin note: text overlap with arXiv:2408.02309
- Published
- 2024