Observing an accretion disk inside a wormhole shadow

The paper considers the problem of the possibility of observing an accretion disk through the throat of the Ellis-Bronnikov-Morris-Thorne wormhole. It is shown that this image has a complex structure and is fundamentally different from the image of an accretion disk around a black hole. Images of the accretion disk are presented at various angles between the plane of the disk and the observer's line of sight.