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.
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Pith papers citing it
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astro-ph.HE 3representative citing papers
NICER data from 4U 1630-47's 2025 outburst show QPOs tied to disk parameter shifts in the rising phase and a weak QRM near peak resembling reduced heartbeat variability.
Type-C QPOs in MAXI J1348-630 exhibit stable ~7 Hz frequency despite intensity changes, hard rms spectra with peaks above 20 keV, and opposite hysteresis in frequency-flux relations between main and mini-outbursts.
citing papers explorer
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Optical polarimetry of the accreting black hole X-ray binary Swift J1727.8$-$1613 over the state transition and radio ejections
Optical polarimetry shows intrinsic ~0.3% polarization from scattering in the accretion disk wind of Swift J1727.8-1613, with polarization angle offset from the jet indicating black hole spin-orbit misalignment.
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Timing and spectral analysis of the 2025 outburst of 4U 1630$-$47 with \textit{NICER}
NICER data from 4U 1630-47's 2025 outburst show QPOs tied to disk parameter shifts in the rising phase and a weak QRM near peak resembling reduced heartbeat variability.
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The full evolution of the type-C QPO in MAXI J1348-630 revealed by Insight-HXMT
Type-C QPOs in MAXI J1348-630 exhibit stable ~7 Hz frequency despite intensity changes, hard rms spectra with peaks above 20 keV, and opposite hysteresis in frequency-flux relations between main and mini-outbursts.