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Fig. 10

image

Cloudlet in an elliptical orbit. In the perifocal frame, with Sgr A* in one of the ellipse focus, the position the cloudlet is determined by the true anomaly angle f. In the plane of the sky, the velocity measured along the line-of-sight depends on the argument of periapsis ω and on the inclination angle i between the orbit and the sky planes.

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