Dramatic Drop in the X-Ray Polarization of Swift J1727.8โ1613 in the Soft Spectral State
Dramatic Drop in the X-Ray Polarization of Swift J1727.8โ1613 in the Soft Spectral State
Abstract Black hole X-ray binaries exhibit different spectral and timing properties in different accretion states. The X-ray outburst of a recently discovered and extraordinarily bright source, Swift J1727.8โ1613, has enabled the first investigation of how the X-ray polarization properties of a source evolve with spectral state. The 2โ8 keV polarization โฆ