Large energy-dependent X-ray polarization degree is detected by the Imaging
X-ray Polarimetry Explorer (IXPE) in the high-soft emission state of the
black hole X-ray binary 4U 1630–47. The highly significant detection (at
≈50σ confidence level) of an unexpectedly high polarization,
rising from ∼6% at 2 keV to ∼10% at 8 keV, cannot be easily
reconciled with standard models of thin accretion discs. In this work we
compare the predictions of different theoretical models with the IXPE data
and conclude that the observed polarization properties are compatible with a
scenario in which matter accretes onto the black hole through a thin disc,
covered by a partially-ionized atmosphere flowing away at mildly relativistic
velocities.
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关键词
Polarimetry,X-ray astronomy,Stellar mass black holes,Accretion