Optical polarimetry shows intrinsic ~0.3% polarization from scattering in the accretion disk wind of Swift J1727.8-1613, with polarization angle offset from the jet indicating black hole spin-orbit misalignment.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Type-C QPOs in Swift J1727.8-1613 exhibit energy-dependent rms-frequency relations with a common break at 4 Hz, indicating a change in accretion geometry.
citing papers explorer
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Optical polarimetry of the accreting black hole X-ray binary Swift J1727.8$-$1613 over the state transition and radio ejections
Optical polarimetry shows intrinsic ~0.3% polarization from scattering in the accretion disk wind of Swift J1727.8-1613, with polarization angle offset from the jet indicating black hole spin-orbit misalignment.
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An Insight-HXMT View of the Evolution of the Type-C Quasiperiodic Oscillation during the Flaring State of Swift J1727.8-1613
Type-C QPOs in Swift J1727.8-1613 exhibit energy-dependent rms-frequency relations with a common break at 4 Hz, indicating a change in accretion geometry.