Recent X-ray polarimetric data on the prototypical black hole X-ray binary Cyg X-1 from the Imaging X-ray Polarimetry Explorer present tight constraints on accretion geometry in the hard spectral state. Contrary to general expectations of a low, ≲1% polarization degree (PD), the observed average PD was found to be a factor of 4 higher. Aligned with the jet position angle on the sky, the observed polarization favors geometry of the X-ray emission region stretched normally to the jet in the accretion disk plane. The high PD is, however, difficult to reconcile with the low orbital inclination of the binary
- Award ID(s):
- 2003828
- PAR ID:
- 10325290
- Date Published:
- Journal Name:
- Journal of Magnetism and Magnetic Materials
- Volume:
- 537
- Issue:
- C
- ISSN:
- 0304-8853
- Page Range / eLocation ID:
- 168234
- Format(s):
- Medium: X
- Sponsoring Org:
- National Science Foundation
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