Detecting Black Hole accretion disc

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Detecting the plane of a black hole's accretion disc can be inferred from the orbital plane of a binary system, as the outer disc aligns with this plane. The inner disc, however, aligns with the equatorial plane of the spinning black hole due to the Bardeen-Petterson effect, which is influenced by frame dragging. Iron K alpha line fluorescence from the inner region of the accretion disc can provide additional data, as it is linked to the x-ray emissions from the disc. Understanding the relationship between the binary's orbital plane and the accretion disc can help identify the black hole's pole and potential jet regions. The consistency of observations with these theoretical models remains a critical question in astrophysics.
zankaon
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How might one detect the plane of an accretion disc of a Black Hole? Might it just be assumed, by the orbital plane of a BH binary system? http://en.wikipedia.org/wiki/Accretion_disc"
 
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The outer disk might well be aligned with the orbital plane, but the inner disk should be aligned with the equatorial plane of the spinning (Kerr) black hole. It's called the Bardeen-Petterson effect and it's due to frame dragging.

Jim Graber
 
BH binary etc.

One has Iron K alpha line fluorescence http://http://en.wikipedia.org/wiki/X-ray_fluorescence" reverberation from a surface, with an initial x-ray source. The iron line emission is supposed to be from inner aspect of accretion disk. So if one knows the orbital plane of a binary, then roughly (via Bardeen Peterson effect i.e. gravitomagnetic i.e. frame dragging from rotation) one would know approximately BH accretion disk plane, and hence approximate orthogonal pole of BH, which would supposedly correspond to any jet detection region. So interrelatedness; but are observations consistent enough with such description?
 
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