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.
Title resolution pending
3 Pith papers cite this work. Polarity classification is still indexing.
3
Pith papers citing it
representative citing papers
Long-term Swift and MAXI observations reveal step-like shifts in Type I outburst orbital phases of GRO J1008-57 that coincide with Type II outbursts, interpreted as cycles of disk depletion and reconstruction.
Simulations show that iterative source removal and maximum likelihood decoding can recover point-source positions and fluxes from 1.5D coded-aperture data with 5-arcmin resolution in one axis and 5-degree resolution in the other.
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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Temporal evolution of the circumstellar disk orientation in the transient X-ray pulsar GRO J1008-57
Long-term Swift and MAXI observations reveal step-like shifts in Type I outburst orbital phases of GRO J1008-57 that coincide with Type II outbursts, interpreted as cycles of disk depletion and reconstruction.
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Simulations of a 2 x 1.5D coded aperture camera for X-ray astronomy
Simulations show that iterative source removal and maximum likelihood decoding can recover point-source positions and fluxes from 1.5D coded-aperture data with 5-arcmin resolution in one axis and 5-degree resolution in the other.