2025/08/07 by Unnati Kashyap, Thomas J. Maccarone, Kashyap, Unnati +9 · 1 citation
Physics and Astronomy · Engineering · #Astrophysical Phenomena and Observations #Mechanics and Biomechanics Studies #Astronomical Observations and Instrumentation
paper · pdf · doi:10.48550/arxiv.2508.05763
We report the X-ray and radio polarization study of the neutron star (NS) low-mass X-ray binary (LMXB) GX 13+1 using the Imaging X-ray Polarimetry Explorer (IXPE) and Very Large Array (VLA). Simultaneous Neutron Star Interior Composition Explorer (NICER) observations show that the source was in parts of the Z state during our IXPE observations, exhibiting moderate changes in the hardness intensity diagram. The source exhibits X-ray dips in the light curve along with hints of polarization swings between the dip and non-dip states. The X-ray spectro-polarimetry results suggest a source geometry comprising an accretion disk component representing the softer disk emission, along with a blackbody representing the harder emission from the boundary layer (BL) or a spreading layer (SL). We investigate the geometry of GX 13+1 by considering our X-ray and radio polarization findings.