Frederick Lamb predicted that motions arising from it would result in weak sidebands on the oscillations produced by neutron stars in binary systems; the strong oscillations were observed in 1996 by the Rossi Explorer satelite.
One result of this effect is the orbital precession of X-ray emitting gas near black holes, resulting in specific X-ray emission peaks. Frederick Lamb predicted that motions arising from it would result in weak sidebands on the oscillations produced by neutron stars in binary systems; the strong oscillations were observed in 1996 by the Rossi Explorer satelite. The decay of oscillations arising from it is known as the Bardeen-Petersen effect, and in calculations of the precession frequency in gravitational systems, this term appears as del cross h. Also known as frame dragging, FTP, identify this effect of general relativity in which the orbit of a small body around a large rotating one is perturbed by the rotation.
One result of this effect is the orbital precession of X-ray emitting gas near black holes, resulting in specific X-ray emission peaks.
{Lense}-{Thirring effect} (accept {frame dragging} before it’s mentioned)